The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal in shape with a yellow hue. It exhibits a concentrated central bulge that fades outward, lacking discernible spiral arm structures or significant dust lanes. The light profile suggests a relatively old stellar population, likely dominated by evolved stars, with a low ongoing star formation rate. There is no indication of recent major merger activity, although the presence of some minor disturbance cannot be ruled out. The galaxy is of intermediate size.
