The galaxy presents as a smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing largely rounded in shape. The central region appears brighter and more condensed than its diffuse outer regions, gradually fading into the background sky. The galaxy displays a distinct yellowish-orange color profile, which may be indicative of an older stellar population, or the presence of dust. There is no visually discernible evidence of spiral arm structure, bar features, or any significant tidal disturbances that would suggest a recent or ongoing merger event. The overall impression is that of a quiescent, relatively undisturbed galaxy.
