The galaxy presents as a relatively smooth, centrally concentrated elliptical, with a slight elongation. The core region appears brighter and more compact. There are no prominent spiral arms or significant dust lanes visible. Color gradients suggest bluer hues toward the central region, indicating a potential concentration of younger stars, although the overall color is fairly uniform. The light profile appears to follow a Sersic profile, suggesting that the light is distributed smoothly and regularly throughout the galaxy. There is a slight asymmetry, indicative of a minor disturbance or recent interaction with another galaxy. 