NGC 1277 is a lenticular galaxy located approximately 220 million light-years away in the constellation Perseus. It is notable for its unusual characteristics, including a high concentration of stars and a massive central black hole, which is estimated to be about 17 billion times the mass of the Sun. Discovered in 1876 by astronomer Édouard Stephan, NGC 1277 is part of the Perseus Cluster of galaxies. Its unique structure and composition provide valuable insights into galaxy formation and evolution, making it a subject of interest for astronomers studying the dynamics of galaxies in the universe.