The galaxy presents as a smooth, elliptical-like structure. It exhibits a bright, concentrated central bulge that dominates its overall luminosity. The light profile fades gradually from the core outwards. The galaxy appears relatively undisturbed, showing no signs of recent major mergers or tidal interactions. It has a slight elongation, deviating modestly from perfect circularity. A subtle color gradient is noticeable, with a yellow-orange hue indicative of an older stellar population throughout the galaxy. There is little evidence of significant ongoing star formation.
