NGC 4797 is a barred spiral galaxy located approximately 60 million light-years away in the constellation Centaurus. It is part of the Centaurus Cluster, which contains many other galaxies and is one of the closest galaxy clusters to Earth. This galaxy has a diameter of about 100,000 light-years and is notable for its bright central region and well-defined spiral arms. NGC 4797 is classified as a type SBc galaxy, indicating it has a prominent bar structure and loose spiral arms, making it an interesting subject for astronomers studying galaxy formation and evolution.