The galaxy presents as a smooth, centrally concentrated object with a generally elliptical morphology. It appears relatively undisturbed, showing no obvious signs of a major merger event. The light profile indicates a primarily spheroidal structure, likely an elliptical galaxy or a lenticular galaxy seen face-on. The galaxy exhibits a color gradient, with a yellowish core transitioning to a redder halo region. This color suggests an older stellar population, particularly in the central bulge. There are no indications of significant dust lanes or spiral arm structures. The overall appearance suggests a galaxy that is relatively quiescent in terms of star formation activity.
