The galaxy presents as a slightly elongated, centrally concentrated object. It exhibits a smooth, luminous profile, suggestive of an elliptical morphology or a lenticular galaxy seen at a moderate inclination. A subtle color gradient is observed, with the central region appearing whiter and potentially hotter, surrounded by a cooler, bluer halo. There is a faint indication of a possible disk. No strong dust lanes or active star-forming regions are readily apparent, which is consistent with a more evolved stellar population. There is a hint of some minor disturbance in the outer edges. The galaxy appears relatively isolated.
