The galaxy appears as a centrally concentrated, largely featureless object with a smooth light distribution. It exhibits a nearly circular morphology, showing minimal deviation from a rounded shape. Color gradients are subtle; the core appears slightly more yellow-orange, suggesting an older stellar population compared to the faint, diffuse outer regions which exhibit a slight greenish tint. There is no discernible spiral structure, bar, or evidence of significant dust lanes. The overall appearance indicates a system that has largely completed its morphological evolution, exhibiting characteristics consistent with an elliptical galaxy or a lenticular galaxy seen face-on. There is no obvious indication of tidal disturbances or ongoing merger activity.
