NGC 1016
NGC 1016 is a barred spiral galaxy located approximately 55 million light-years away in the constellation Hydra. It was discovered by the astronomer John Herschel in 1834 and is part of the Hercules Cluster.
This galaxy has a diameter of about 100,000 light-years and features a bright central bar structure. NGC 1016 is notable for its active star formation regions, which contribute to its vibrant appearance. Observations of this galaxy help astronomers understand the dynamics and evolution of spiral galaxies in the universe.