The galaxy presents a smooth, elliptical morphology. The central region exhibits a concentrated, bright core, transitioning outward to a less luminous, more diffuse halo. The color profile suggests a relatively evolved stellar population, with a reddish hue dominating the central region, likely indicative of older stars. The outer regions show a subtle shift towards bluer tones, implying the presence of younger, though not intensely active, star formation. There is no evidence of significant spiral arm structure, strong tidal features, or ongoing major mergers. The galaxy appears relatively undisturbed and quiescent.
