The galaxy presents as a relatively smooth, centrally concentrated object with a flattened, elliptical morphology. The central region exhibits a bright, high-surface-brightness core, suggesting the presence of a significant stellar population. The galaxy displays a distinct color gradient, with the core appearing more yellow-white, and the outer regions exhibiting a bluer hue. This color difference potentially indicates differing stellar populations, with older, redder stars dominating the core and younger, bluer stars more prevalent in the outer regions. A faint disk-like structure seems to be present, oriented horizontally across the frame. There is no immediately apparent evidence of major mergers or significant tidal disturbances affecting the galaxy's structure, although there are some hints of minor disturbances.
