The galaxy presents as a predominantly elliptical morphology, exhibiting a smooth, centrally concentrated light profile. The core region is characterized by a bright, yellowish-orange hue, suggestive of an older stellar population. The galaxy exhibits a generally round shape, with a slight elongation.

There is some visual evidence of a minor disturbance along its edge.

The overall color gradient indicates a likely lack of significant ongoing star formation within the galaxy's disk, implying a transition to a passive, more evolved state.
