NGC 124 is a barred 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 124 has a bright central bar structure and exhibits a mix of young and old stars, making it an interesting object for astronomers. The galaxy spans about 100,000 light-years in diameter and is notable for its distinct spiral arms. Observations of NGC 124 contribute to our understanding of galaxy formation and evolution, particularly in relation to other galaxies in the Hubble Sequence.