NGC 4750
NGC 4750 is a barred spiral galaxy located approximately 60 million light-years away in the constellation Centaurus. It was discovered by the astronomer John Herschel in 1834. The galaxy is notable for its distinct bar structure, which is a common feature in many spiral galaxies.
This galaxy is part of the Centaurus group, a collection of galaxies that includes several other notable members. NGC 4750 has an apparent magnitude of about 11.5, making it a faint object that requires a telescope for observation. Its unique morphology provides valuable insights into the formation and evolution of galaxies.