The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, potentially indicative of an older stellar population. The galaxy displays a radial color gradient, appearing more yellow/red in the central regions, suggesting the dominance of older, cooler stars there. The outer regions appear slightly bluer, potentially indicating a small amount of ongoing star formation. The overall shape is somewhat elongated, although tending more towards circularity than a highly elongated ellipsoid. There are no apparent signs of spiral arms or significant dust lanes. The galaxy shows minimal signs of interaction or recent merger activity.
