The galaxy presents a largely homogenous, elliptical morphology, with a smooth light distribution indicating an older stellar population and a lack of significant dust lanes. The radial profile shows a concentrated central bulge that gradually fades outward into a diffuse halo. The colour gradient exhibits a subtle reddening toward the centre. This suggests a concentration of older, redder stars in the core of the galaxy. There is no indication of spiral arms or other distinct features, such as star-forming regions, which is consistent with an evolved stellar population. The galaxy appears relatively undisturbed, showing no obvious signs of recent mergers or tidal interactions.
