The galaxy presents as a relatively smooth, centrally concentrated structure. The core exhibits a bright, somewhat diffuse glow that fades outward. The shape is generally elliptical but not perfectly round, leaning towards an intermediate form. There is no clearly defined disk or spiral structure visible; the overall impression is that of a spheroidal galaxy. The color profile suggests a dominant population of older stars with a reddish hue in the central region, surrounded by a slightly bluer, but still relatively faint, halo. No strong signs of ongoing major mergers or tidal disturbances are immediately apparent.
