The galaxy presents a generally smooth, elliptical morphology. It has a concentrated, bright core that gradually fades into a diffuse halo. The color profile suggests an aging stellar population, with a redder hue dominating the central region, transitioning to slightly bluer tones in the outer regions. There appears to be no significant dust lane obscuration or prominent spiral arm structure, indicating a relatively undisturbed system. The overall structure appears largely spheroidal with no signs of ongoing major mergers or tidal disturbances.
