The galaxy presents as a centrally concentrated object with an elliptical morphology. A smooth light distribution is observed across the majority of the galaxy's surface. The central region exhibits a yellowish-orange hue, suggestive of an older stellar population dominating the core. Moving outward from the center, the color gradually transitions to a greenish tint, possibly indicating the presence of younger stars. There is no obvious spiral structure or significant dust lane apparent in this image. The overall appearance is relatively undisturbed, showing no strong signs of on-going major mergers or tidal interactions.
