NGC 4709
NGC 4709 is a barred spiral galaxy located in the constellation Centaurus. It is approximately 60 million light-years away from Earth and is part of the Centaurus group of galaxies. NGC 4709 has a bright core and distinct spiral arms, making it an interesting object for astronomers.
Discovered by the astronomer John Herschel in 1834, NGC 4709 is notable for its relatively high surface brightness. It is often studied to understand the structure and dynamics of spiral galaxies, contributing to our knowledge of galaxy formation and evolution in the universe.