NGC 4540 is a spiral galaxy with type 1 Seyfert activity located about 64 million light-years away in the constellation Coma Berenices. NGC 4540 was discovered by astronomer William Herschel on March 21, 1784 and is a member of the Virgo Cluster.
NGC 4326 is a barred spiral galaxy with a ring located about 330 million light-years away in the constellation Virgo. It was discovered by astronomer William Herschel on April 13, 1784, who described it as "vF, S, R, bM, 1st of 3". It is a large galaxy, with a diameter of around 200,000 ly (61 kpc) making it nearly twice the size of the Milky Way. NGC 4326 is also classified as a LINER galaxy. Despite being listed in the Virgo Cluster catalog as VCC 623, it is not a member of the Virgo Cluster but instead a background galaxy.
NGC 4333 is a barred spiral galaxy with a ring structure located about 330 million light-years away in the constellation Virgo. It was discovered by astronomer William Herschel on April 13, 1784, who described it as "F, pS, R, bM, 2nd of 3". NGC 4333 is also classified as a LINER galaxy. Despite being listed in the Virgo Cluster catalog as VCC 637, it is not a member of the Virgo Cluster but instead a background galaxy.
IC 3528 is a Seyfert 1.5 type spiral galaxy with X-ray emission located 660 million light-years away in the constellation of Coma Berenices. It lies near to spiral galaxy NGC 4540, although the two of them are quite far. The object was discovered by Royal Harwood Frost on May 7, 1904. Although listed as a member in the Virgo Cluster Catalogue as VCC 1593, it is not a member of the Virgo cluster but a background galaxy.
IC 4617 is a type Sbc spiral galaxy located in the Hercules constellation. It is located 553 million light-years from the Solar System and has an estimated diameter of 115,000 light-years thus making it slightly larger compared to the Milky Way. The galaxy was discovered by American astronomer, Edward Emerson Barnard or E. E. Barnard although no date of discovery was confirmed. IC 4617 is a member of Abell 2199 and happens to lie near towards the globular cluster, Messier 13.
NGC 3754 is a small barred spiral galaxy located in Leo. It is located 447 million light-years away from the Solar System and was discovered on April 5, 1874, by Ralph Copeland.
IC 1192 is an edge-on barred spiral galaxy located in Hercules. It is located 543 million light-years from the Solar System and has a diameter of approximately 90,000 light-years. IC 1192 was discovered by Stephane Javelle on August 13, 1892. It is a member of the Hercules Cluster.
IC 2759 is a small type E elliptical galaxy located in the constellation of Leo. It is located 350 million light-years away from the Solar System and was discovered on April 24, 1897, by Guillaume Bigourdan. Sometimes IC 2759 is confused with the spiral galaxy, PGC 34882 which is located south of the galaxy.
NGC 7222 is a large barred spiral galaxy with a ring structure, located in the constellation Aquarius. It is located 570 million light-years away from the Solar System and was discovered by German astronomer, Albert Marth on August 11, 1864.
IC 848 is a type Sbc barred spiral galaxy located in Coma Berenices. Its redshift is 0.053077 which corresponds the galaxy to be located 727 million light-years away from Earth. IC 848 has an apparent dimension of 0.80 x 0.6 arcmin, meaning it is about 170,000 light-years across. It was discovered by Stephane Javelle on July 22, 1892, which was described per Dreyer as "extremely faint, very small and difficult".
IC 3278 known as PGC 40345, is a large type SBbc spiral galaxy located in Coma Berenices. Its redshift is 0.093851, meaning IC 3278 is 1.29 billion light-years away from Earth, which given its apparent dimensions of 0.80 x 0.6 arcmin, means IC 3278 is 301,000 light-years across. The galaxy was discovered on March 23, 1903, by Max Wolf. Together with two lenticular galaxies, IC 3278 NED01 and IC 3278 NED02, they form a galaxy triplet bearing its same name. According to a study which was conducted by Takase and Miyauchi-Isobe, IC 3278 can be considered an ultraviolet-excess galaxy as it is detected on multi-color plates which was taken via a Kiso Schmidt telescope for 10 survey fields.
IC 3078 is a spiral galaxy with a ring structure located in Virgo. Its redshift is 0.066148, meaning IC 3078 is located 905 million light-years from Earth. With an apparent dimension of 0.50 x 0.5 arcmin, IC 3038 is about 133,000 light-years across. It was discovered by Royal Harwood Frost on May 7, 1904 and is listed in the Virgo Cluster catalogue as VCC 174. However, it is not a member of the Virgo Cluster, but instead a background galaxy.
IC 4539 is a type SABb intermediate spiral galaxy located in Corona Borealis. Its redshift is 0.061307, which corresponds IC 4539 to be 845 million light-years from Earth. It has an apparent dimension of 0.40 x 0.4 arcmin, meaning the galaxy is about 95,000 light-years across. IC 4539 was discovered by Stephane Javelle on June 23, 1903, who found it "as faint, small, round with a very brighter middle."
IC 923 is a lenticular galaxy located in Ursa Major. Its redshift is 0.069243 which means the galaxy is 954 million light-years from Earth. IC 923 has apparent dimensions of 0.50 x 0.2 arcmin, meaning it is approximately 139,000 light-years across. IC 923 was discovered in June 1892, by Edward Emerson Barnard and is a member of galaxy group, V1CG 588.
IC 2734 is a type SBc barred spiral galaxy seen edge-on, and located in the constellation Leo. Its redshift is 0.078901, which corresponds IC 2734 to be located 1.09 billion light-years from Earth. The galaxy has an apparent dimension of 0.60 x 0.2 arcmin, meaning it is approximately 190,000 light-years across. IC 2734 was discovered on March 27, 1906, by astronomer, Max Wolf.
IC 4160, also known as PGC 1677859, is a spiral galaxy located in Coma Berenices. Its redshift is 0.061443, which corresponds IC 4160 to be 846 million light-years from Earth. It has an apparent dimension of 0.40 x 0.2 arcmin, meaning the galaxy is 99,000 light-years across. IC 4160 was discovered by Max Wolf on January 27, 1904.
IC 2754 is a type Sc spiral galaxy located in the constellation Leo. Its redshift is 0.070479, which corresponds to IC 2754 being 970 million light-years from Earth. It has an apparent dimension of 0.50 x 0.2 arcmin, which means IC 2754 is 141,000 light-years across. IC 2754 was discovered on March 27, 1906, by Max Wolf.
IC 2839, known as PGC 3472295, is a spiral galaxy located in the constellation Leo. Its redshift is 0.065734, which corresponds to the galaxy being located 906 million light-years from Earth. IC 2839 has an apparent dimension of 0.30 x 0.1 arcmin, meaning it spans 79,000 light-years across. The galaxy was discovered on March 27, 1906, by Max Wolf.
IC 3447 is a type Sc barred spiral galaxy located in the constellation Virgo. It has a redshift of 0.092479, which means IC 3447 is 1.27 billion light-years from Earth, making it one of the furthest objects in the Index Catalogue. The galaxy has apparent dimensions of 0.30 x 0.3 arcmin, which means IC 3447 is 111,000 light-years across. It was discovered by Royal Harwood Frost on May 10, 1904.
NGC 3950 is an elliptical galaxy of type E, in Ursa Major. Its redshift is 0.074602, meaning NGC 3950 is 1.03 billion light-years or 316 Mpc from Earth, which is within the Hubble distance values. This high redshift makes NGC 3950 one of the furthest New General Catalogue objects.
