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 star-forming regions. NGC 1024 is part of a larger group of galaxies and is often studied to understand the dynamics and evolution of spiral galaxies in the universe.