NGC 126 is a spiral galaxy located in the constellation of Perseus. It is part of the Abell 426 galaxy cluster and is approximately 250 million light-years away from Earth. NGC 126 has a bright core and exhibits a well-defined spiral structure, making it an interesting object for astronomers. The galaxy is classified as a type SAB, indicating it has a weakly barred spiral structure. Observations of NGC 126 contribute to our understanding of galaxy formation and evolution, particularly in the context of galaxy clusters like Abell 426.