NGC 4995 is a barred spiral galaxy located approximately 50 million light-years away in the constellation Centaurus. It is part of the Centaurus Group, which contains several other galaxies. NGC 4995 is notable for its bright core and well-defined spiral arms, making it an interesting subject for astronomers. This galaxy is classified as a type SBc, indicating its spiral structure with a central bar. Observations of NGC 4995 have provided insights into galaxy formation and evolution, contributing to our understanding of the universe's structure and the dynamics of galactic interactions.