NGC 4699 is a barred spiral galaxy located approximately 50 million light-years away in the constellation Centaurus. It is part of the Centaurus Cluster, which contains many other galaxies. NGC 4699 is notable for its bright core and well-defined spiral arms, making it an interesting subject for astronomers studying galaxy formation and structure. Discovered by John Herschel in 1834, NGC 4699 has a visual magnitude of about 11.5, making it faintly visible through small telescopes. Its distance and characteristics provide valuable insights into the dynamics of galaxies and their interactions within clusters.