The galaxy presents as an elliptical morphology, with a smooth, relatively featureless appearance. It exhibits a concentrated central bulge that gradually fades into a more diffuse halo. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the overall appearance. There is no discernible evidence of spiral arms or significant dust lanes. The overall shape appears generally round, with no obvious signs of tidal disturbances or ongoing merger activity.
