The galaxy presents as a centrally concentrated, elliptical morphology. The core exhibits a high degree of smoothness and a yellow-orange color, suggestive of an older stellar population with minimal ongoing star formation. The galaxy appears to be relatively undisturbed, showing no signs of major mergers or significant tidal disruptions. There may be a slight elongation in the shape, but the overall form remains fairly regular. The absence of prominent spiral arms or distinct dust lanes further supports the classification as an elliptical galaxy.
