NGC 4740
NGC 4740 is a barred spiral galaxy located in the constellation Centaurus. It is approximately 65 million light-years away from Earth and is part of the Centaurus galaxy cluster. NGC 4740 has a distinct structure characterized by its bright central bar and spiral arms, making it an interesting subject for astronomers.
This galaxy was first cataloged by the astronomer John Herschel in 1834. NGC 4740 is notable for its relatively high surface brightness and is often studied to understand the formation and evolution of spiral galaxies. Its features provide insights into the dynamics of galactic structures.