NGC 2474 is a barred spiral galaxy located approximately 100 million light-years away in the constellation Hydra. It is classified as a type SBc galaxy, which means it has a prominent bar structure and loose spiral arms. The galaxy spans about 70,000 light-years in diameter and is part of the Laniakea Supercluster. NGC 2474 is notable for its bright central region and active star formation, making it an interesting subject for astronomers studying galaxy evolution and structure.