The galaxy presents as a primarily smooth, elliptical-like structure with a concentrated central bulge. The core exhibits a yellowish-orange hue, suggestive of an older stellar population. Fainter, reddish-colored regions extend outward from the central bulge. These regions indicate the presence of dust lanes or possibly areas of on-going, but limited, star formation. The galaxy exhibits some level of disturbance or asymmetry, particularly in the outer regions, which may be indicative of a past or ongoing minor merger event. The overall morphology is not perfectly spherical, tending towards a slightly elongated shape.
