The galaxy presents as a single, largely featureless elliptical structure. It exhibits a smooth, centrally concentrated luminosity profile, with a gradual decrease in brightness extending outwards from a bright nucleus. The shape appears generally ellipsoidal, showing a slight elongation rather than perfect circularity. The light distribution suggests a relatively old stellar population, consistent with a low star formation rate and an absence of prominent dust lanes or spiral arms. The galaxy appears undisturbed, lacking any obvious signs of recent mergers or tidal interactions. Color gradients are subtle, with a slightly redder hue towards the central region, indicating a potential concentration of older, redder stars in the core.
