The galaxy presents as a centrally concentrated, elliptical system with a smooth light profile. The core region exhibits a golden-yellow hue, suggesting an older stellar population with a paucity of ongoing star formation. There is a distinct lack of blue light associated with younger, hotter stars or star-forming regions. The galaxy appears relatively undisturbed, showing no obvious signs of recent major mergers or tidal interactions, although closer inspection reveals some possible minor disturbances in the very outer regions. It exhibits a high degree of rotational symmetry, appearing nearly circular in projection.
