The galaxy presents a predominantly smooth and rounded morphology. The light profile appears centrally concentrated, suggestive of an elliptical galaxy type. The core exhibits a yellowish-orange hue, possibly indicating an older stellar population dominating the central region. Fainter greenish light is around the edges of the galaxy, maybe indicating some ongoing star formation. There are no visually apparent spiral arm structures or significant dust lanes. No major merging event can be observed. Any merging events appear to be minor.