The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be elliptical in shape, with a high degree of central bulge concentration surrounded by a more diffuse, extended halo. The color profile suggests an aging stellar population with a higher concentration of older, redder stars in the central bulge which transitions to a bluer halo. There is a hint of a slight disturbance in the outer halo, but no major signs of tidal features or ongoing major mergers are visible. The overall morphology points towards a relaxed system that may be undergoing minor interactions.
