NGC 514

NGC 514 is a barred spiral galaxy located approximately 100 million light-years away in the constellation Pisces. It was discovered on October 16, 1784, by the astronomer William Herschel.

NGC 514 is classified as a SAB(rs)c galaxy, where "SAB" indicates a weak bar structure, "(rs)" denotes a weak inner ring or pseudoring feature, and "c" signifies loosely wound spiral arms. The galaxy exhibits active star formation, particularly in its spiral arms, which are rich in gas and dust.

It is a relatively isolated galaxy, meaning it is not part of a large galaxy cluster or group. Its size is estimated to be around 150,000 light-years in diameter, making it somewhat larger than the Milky Way.

Studies of NGC 514 have contributed to our understanding of spiral galaxy structure, star formation processes, and the distribution of matter in the universe. Its relative proximity and bright appearance make it a popular target for amateur and professional astronomers alike.