NGC 4789 is a barred spiral galaxy located approximately 60 million light-years away in the constellation Coma Berenices. It is part of the Virgo Cluster and is notable for its bright core and well-defined spiral arms, which are characteristic features of spiral galaxies. Discovered by the astronomer William Herschel in 1785, NGC 4789 has an apparent magnitude of about 11.5, making it a faint object that requires a telescope to observe. Its structure and composition provide valuable insights into the formation and evolution of galaxies in the universe.