NGC 123 is a spiral galaxy located in the constellation of Cetus. It is approximately 70 million light-years away from Earth and is part of the Peculiar Galaxy group. NGC 123 is notable for its bright core and well-defined spiral arms, which are characteristic features of spiral galaxies. Discovered in the 19th century, NGC 123 has been the subject of various astronomical studies. Its structure and composition provide insights into galaxy formation and evolution. Observations of NGC 123 contribute to our understanding of the universe and the dynamics of galaxies within it.