NGC 598
NGC 598 is a spiral galaxy located in the constellation of Hydra. It is part of the Messier 100 group and is approximately 60 million light-years away from Earth. NGC 598 has a diameter of about 100,000 light-years and contains billions of stars, along with gas and dust that contribute to star formation.
Discovered by William Herschel in 1785, NGC 598 is notable for its well-defined spiral structure. It is classified as a type Sc spiral galaxy, which means it has tightly wound arms and a prominent central bulge. Observations of NGC 598 provide valuable insights into the formation and evolution of galaxies.