NGC 4489 is a dwarf elliptical galaxy located about 60 million light-years away in the constellation of Coma Berenices. It was discovered by astronomer William Herschel on March 21, 1784. NGC 4489 is a member of the Virgo Cluster.
NGC 4633 is a spiral galaxy located about 70 million light-years away in the constellation of Coma Berenices. It is interacting with the nearby galaxy NGC 4634. NGC 4633 was discovered by astronomer Edward D. Swift on April 27, 1887. It was rediscovered on November 23, 1900, by astronomer Arnold Schwassmann and was later listed as IC 3688. NGC 4633 is a member of the Virgo Cluster.
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 4222 is an edge-on spiral galaxy located about 60 million light-years away in the constellation Coma Berenices. It was discovered by astronomer William Herschel on April 8, 1784 and is often misidentified as IC 3087. NGC 4222 is a member of the Virgo Cluster and is a companion of NGC 4216 which lies about 180,000 ly (56 kpc) away. Despite this, the two galaxies are not interacting.
NGC 4895 is a lenticular galaxy located 330 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer Heinrich d'Arrest on May 5, 1864 and is a member of the Coma Cluster.
NGC 4056 is an elliptical galaxy located about 340 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer Albert Marth on March 18, 1865 and is a member of the NGC 4065 Group.
NGC 4359 is a dwarf barred spiral galaxy seen edge-on that is about 56 million light-years away in the constellation Coma Berenices. It was discovered by astronomer William Herschel on March 20, 1787. It is a member of the NGC 4274 Group, which is part of the Coma I Group or Cloud.
IC 3505 is a barred spiral galaxy located 640 million light-years away from the Solar System in the Coma Berenices constellation. With an apparent size of 0.95 by 0.35 arcmin, IC 3505 has an estimated diameter of 170,000 light-years, making it slightly larger compared to the Milky Way. It is categorized as a LINER galaxy with an active galactic nucleus emitting weak emission-lines.
IC 3482 is a type Sb spiral galaxy in the Coma Berenices constellation. It is located 850 million light-years away from the Solar System. IC 3482 has an apparent size of 0.4 x 0.15 arcmin, meaning it has estimated diameter of 140,000 light-years. IC 3482 was discovered on March 23, 1903, by German astronomer pioneer, Max Wolf. It is located at right ascension of (12:33:01.00) and declination of (27:49:49:10), and has a surface brightness of magnitude 23.
IC 3789, occasionally known as PGC 1619535, is a type Sbc barred spiral galaxy in the Coma Berenices constellation. It is located 872 million light-years away from the Solar System and has an approximate diameter of 150,000 light-years making it slightly larger than the Milky Way. IC 3789 was discovered on 27 January 1904 by astronomer Max Wolf.
IC 4017 is a type Sbc spiral galaxy with a bar located in Coma Berenices. It is located 2.3 billion light-years away and was discovered on January 27, 1904, by Max Wolf. At the redshift of 0.1773, IC 4017 is the most furthest object in the Index Catalogue and is said to be possibly interacting with its companion.
IC 4040 is a type SABc spiral galaxy with a bar in Coma Berenices. It is located 353 million light-years away from the Solar System and has an estimated diameter of 105,000 light-years making it slightly larger than the Milky Way. IC 4040 was discovered on April 12, 1891, by Guillaume Bigourdan and is a member of the Coma Cluster.
IC 4026 is a type S0 lenticular galaxy with a bar located in Coma Berenices. It is located 315 million light-years away from the Solar System and has an approximate diameter of 70,000 light-years which is less the size of the Milky Way. IC 4026 was discovered on May 11, 1896, by astronomer Hermann Kobold and is a member of the Coma Cluster. It has a surface brightness of 11.99 mag/arcsecs meaning it is a high surface brightness galaxy.
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.
IC 2816 known as PGC 3472124, is a type Sbc spiral galaxy with a ring structure located in the Leo constellation. It is located 878 million light-years from the Solar System and has apparent dimensions of 0.59 x 0.22 arcmin, meaning its diameter is 160,000 light-years across.
IC 3622 also known as PGC 3793395, is a large barred spiral galaxy located in constellation Coma Berenices. It is located 980 million light-years from the Solar System and has a diameter of 175,000 light-years. IC 3622 was discovered by Royal Harwood Frost on May 7, 1904.
IC 4588 is a type E elliptical galaxy located in the constellation Serpens. It is located 729 million light-years from the Solar System and has a dimension of 0.30 x 0.3 arcmin meaning its diameter is 64,000 light-years across. IC 4588 was discovered by Stephane Javelle on July 15, 1903.
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 4163 is a type Sbc peculiar galaxy located in Coma Berenices. Its redshift is 0.064038 which corresponds IC 4163 to be 858 million light-years from Earth. It has an apparent dimension of 0.40' x 0.3' arcmin and was discovered on January 27, 1904, by Max Wolf.
