NGC 1024 is a barred spiral galaxy located approximately 30 million light-years away in the constellation Eridanus. It is classified as a type SBbc galaxy, which means it has a prominent bar structure and loosely wound spiral arms. This galaxy is notable for its bright central region and the presence of several star-forming regions. Observations of NGC 1024 contribute to our understanding of galaxy formation and evolution, particularly in the context of barred spiral galaxies.