3C 305, also known as IC 1065, is a lenticular galaxy located in the constellation Draco. It has an active galactic nucleus and is classified both a Seyfert 2 and radio galaxy The galaxy was discovered by American astronomer Lewis Swift when he came upon it on April 7th, 1888.
IC 3 is a compact elliptical galaxy located approximately 228 million light-years away in the constellation of Pisces. The galaxy was discovered by astronomer Stéphane Javelle on August 27, 1892.
NGC 7013 is a relatively nearby spiral or lenticular galaxy estimated to be around 37 to 41.4 million light-years away from Earth in the constellation of Cygnus. NGC 7013 was discovered by English astronomer William Herschel on July 17, 1784 and was also observed by his son, astronomer John Herschel on September 15, 1828.
NGC 463 is a lenticular galaxy located about 264 million light-years away from Earth in the constellation Pisces. It was discovered by French astronomer Édouard Stephan on December 16, 1871.
NGC 475 is a lenticular galaxy in the constellation Pisces. It is located approximately 750 million light-years from Earth and has a diameter of roughly 125 thousand light-years. NGC 475 was discovered on November 3, 1864 by German astronomer Albert Marth.
NGC 490, also occasionally referred to as PGC 4973 or GC 277, is a lenticular galaxy in the constellation Pisces. It is located approximately 85 million light-years from Earth and was discovered on December 6, 1850, by Irish engineer Bindon Blood Stoney. Although John Dreyer, creator of the New General Catalogue, credits the discovery to astronomer William Parsons, he notes that many of his claimed discoveries were made by one of his assistants. In the case of NGC 490, the discovery was made by Bindon Stoney, who discovered it along with NGC 486, NGC 492 and NGC 500 during his observation of NGC 488.
NGC 499, also occasionally referred to as PGC 5060, IC 1686 or GC 289, is a lenticular galaxy in the constellation Pisces. It is located approximately 197 million light-years from the Solar System and was discovered on 12 September, 1784 by astronomer William Herschel.
NGC 505 is a lenticular galaxy approximately 234 million light-years away from Earth in the constellation of Pisces. It was discovered by German astronomer Albert Marth on October 1, 1864.
NGC 509 is a lenticular galaxy approximately 87 million light-years away from Earth in the constellation of Pisces. It was discovered by German astronomer Albert Marth on October 1, 1864.
NGC 502, also occasionally referred to as PGC 5034 or UGC 922, is a lenticular galaxy in the constellation Pisces. It is located approximately 113 million light-years from the Solar System and was discovered on 25 September 1862 by German astronomer Heinrich Louis d'Arrest. When the Morphological Catalogue of Galaxies was published between 1962 and 1974, the identifications of NGC 502 and NGC 505 were reversed. In reality, NGC 502 is equal to MGC +01-04-041 and not MCG +01-04-043 as noted in the catalogue.
NGC 504, also occasionally referred to as PGC 5084 or UGC 935, is a lenticular galaxy located approximately 189 million light-years from the Solar System in the constellation Pisces. It was discovered on 22 November 1827 by astronomer John Herschel. The object was listed twice in the General Catalogue, precursor of the New General Catalogue, as both GC 291 and GC 292.
NGC 515, also occasionally referred to as PGC 5201 or UGC 956, is a lenticular galaxy located approximately 228 million light-years from the Solar System in the constellation Pisces. It was discovered on 13 September 1784 by astronomer William Herschel.
NGC 517, also occasionally referred to as PGC 5214 or UGC 960, is a lenticular galaxy located approximately 188 million light-years from the Solar System in the constellation Pisces. It was discovered on 13 September 1784 by astronomer William Herschel.
NGC 709 is a lenticular galaxy located 150 million light-years away in the constellation Andromeda. It was discovered by the Irish engineer and astronomer Bindon Blood Stoney on October 28, 1850 and is a member of the galaxy cluster Abell 262.
NGC 530, also known as IC 106, is a lenticular galaxy in the constellation Cetus. It is approximately 226 million light years from the Milky Way and has a diameter of around 100,000 light years. The object was discovered on November 20, 1886, by the American astronomer Lewis A. Swift, who listed it as NGC 530, and rediscovered on November 16, 1887, by Guillaume Bigourdan, who listed it as IC 106.
NGC 6600 is a lenticular galaxy roughly 310 million light-years away in the constellation Hercules. NGC 6600 was discovered in 1864 by Albert Marth. Unlike our own Milky Way, NGC 6600 boasts a tightly wound structure, swirling with stars and gas.
NGC 5790 is a lenticular galaxy located 541 million light-years away in the Boötes constellation. It was discovered on 16 May, 1884 by a French astronomer named Edouard Stephan. The galaxy is approximately 180,000 light-years across. NGC 5790 is a type 2 Seyfert galaxy according to the SIMBAD database.
IC 3971 is a spiral galaxy located approximately 1 billion light-years away from the solar system, in the constellation of Coma Berenices. It was first discovered in January 1904 by German astronomer Max Wolf. According to SIMBAD database, it is a LINER type galaxy with an active nucleus.
IC 3625 is a lenticular galaxy, located in the constellation of Virgo, 990 million light-years away from the solar system. With an apparent size of 0.75 by 0.55 arcmin, IC 3625 has an diameter of 200,000 light years, making it twice the size of the Milky Way. The object was discovered by American astronomer, Royal Harwood Frost on May 10, 1904. Despite listed in the Virgo Cluster catalogue as VCC 1799, it is not a member of the Virgo Cluster but instead a background galaxy.
IC 3441 is a type ES-0 lenticular galaxy with a bar located 880 million light-years away from the solar system in the constellation of Coma Berenices. IC 3441 was discovered on March 23, 1903, by the astronomer Max Wolf and it does not have an active galactic nucleus or an indication of star formation.
