NGC 4799 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 prominent bar structure in its center, which is characteristic of barred spiral galaxies. NGC 4799 is notable for its bright core and well-defined spiral arms, making it an interesting subject for astronomers studying galaxy formation and evolution.