NGC 2150 is an open star cluster located in the constellation Columba. It was discovered by the astronomer John Herschel in 1834 and is situated approximately 1,200 light-years away from Earth. The cluster contains several young stars that are still in the process of forming. The cluster is notable for its relatively high concentration of stars, which are bound together by their mutual gravitational attraction. NGC 2150 is part of a larger group of clusters in the region, contributing to our understanding of stellar formation and evolution in the Milky Way galaxy.