The galaxy exhibits an elliptical morphology, appearing as a smooth, centrally concentrated object. Its shape is elongated, resembling a flattened spheroid, with the major axis oriented roughly horizontally in the image. There is a clear color gradient, with a yellowish-white hue dominating the central region, suggesting an older stellar population. The outer regions display a bluer tint, possibly indicating the presence of younger stars or ongoing star formation, albeit at a modest rate. No distinct spiral arms or prominent dust lanes are visible. There is no immediately visible evidence of any major mergers or tidal disturbances that could be affecting the galaxy. The object appears relatively undisturbed.
