The galaxy presents a disk-like morphology with a prominent, bright central bulge. There is evidence of spiral arm structure, but it is somewhat ill-defined and patchy. The bulge exhibits a yellowish-white hue, suggesting a population of older stars. The disk displays a bluer color, indicating the presence of younger, hotter stars and ongoing star formation. The disk appears somewhat disturbed, potentially indicative of minor interactions or internal processes affecting its structure. Overall, the galaxy exhibits characteristics of a spiral galaxy undergoing active, but possibly declining, star formation.
