The galaxy presents a largely smooth and elliptical morphology. Its overall color profile suggests a population of older stars, exhibiting a yellowish hue which likely indicates a dominance of redder stellar types. There is a centrally concentrated bulge that is significantly brighter than the outer regions. The lack of apparent dust lanes or spiral arm structures is consistent with a classification as an elliptical galaxy. It shows a high degree of radial symmetry. The galaxy exhibits a slight elongation, departing marginally from a perfectly circular shape. There are no signs of recent or ongoing major mergers, although there is a hint of possible minor disturbances in its outer regions. The galaxy is relatively compact.
