This galaxy exhibits a largely smooth morphology, with a dominant central bulge. The shape appears generally elliptical but not perfectly round; it is slightly elongated. There is little evidence of spiral arm structure or significant disk-like features. Color gradients suggest a population of older stars, particularly within the concentrated central bulge. The galaxy shows only minor, if any, signs of disturbance or ongoing mergers. The galaxy seems well-defined, with fairly clear edges given the distance. Overall, this appears to be an evolved galaxy, possibly transitioning towards a more quiescent state.
