The galaxy presents as a moderately bright, elliptical structure. It exhibits a smooth, diffuse profile with a centrally concentrated bulge that dominates the overall light emission. The color profile suggests an older stellar population, with a reddish-yellow hue. There is little evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, showing no strong signs of recent major mergers or tidal interactions. It seems to be a relatively isolated system exhibiting a fairly regular and symmetric shape.
