NGC 2110
NGC 2110 is a barred spiral galaxy located approximately 130 million light-years away in the constellation Columba. It was discovered by the astronomer John Herschel in 1834 and is notable for its bright core and well-defined spiral arms.
This galaxy is classified as a Seyfert galaxy, which means it has an active nucleus that emits strong radiation. NGC 2110 is part of a group of galaxies and is often studied to understand the processes occurring in active galactic nuclei and the formation of galaxies in the universe.