The galaxy presents a largely smooth morphology, with a noticeable central bulge region. It appears elliptical in shape, exhibiting a round to slightly oblong profile. Faint, diffuse extensions emanate from the central region, potentially indicative of a weak disk structure or tidal features, though no strong spiral arm structure is apparent. The color profile suggests a relatively uniform stellar population throughout the galaxy, with a subtle reddening toward the core potentially indicating older stars. There is no compelling evidence for ongoing major mergers or significant disturbances in the galaxy's structure, though minor asymmetries in the outer regions may suggest minor interactions. Overall, the galaxy is characterized by a somewhat centralized brightness distribution with a lack of prominent features.
