NGC 4670 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 cluster of galaxies. NGC 4670 has a distinct structure characterized by its bright central bar and spiral arms, making it an interesting subject for astronomers. Discovered by the astronomer John Herschel in 1834, NGC 4670 is classified as a type SBc galaxy. This classification indicates that it has a prominent bar structure and loosely wound spiral arms. Observations of NGC 4670 contribute to our understanding of galaxy formation and evolution in the universe.