The galaxy presents an elliptical morphology, exhibiting a centrally concentrated luminosity profile that diminishes gradually outwards. It is characterized by a smooth, largely featureless appearance, suggestive of a relatively evolved stellar population. The galaxy displays a moderate ellipticity, appearing somewhat flattened along one axis. There is a color gradient, with the central region appearing more yellow-orange, potentially indicative of older, redder stars dominating the core. The outer regions exhibit a slightly bluer hue, which could point to the presence of a younger, star-forming population, although it's subtle. The overall structure is undisturbed, with no apparent signs of recent major mergers or tidal interactions.
