This galaxy exhibits a distinct spiral structure with loosely wound arms emanating from a moderate-sized central bulge. The color gradients within the spiral arms suggest varying stellar populations and ongoing star formation, with bluer regions indicating younger, hotter stars. The overall morphology indicates that the galaxy is currently undergoing a merger event, characterized by noticeable distortions in its shape and potentially influenced by tidal forces. These interactions may stimulate increased star formation activity within the arms and throughout the galaxy.
