The galaxy presents as a fairly smooth, elliptical structure with a concentrated central bulge. The light distribution appears centrally peaked, transitioning smoothly outwards. The core exhibits a yellowish-white hue, which could be indicative of an older stellar population. A faint, diffuse halo surrounds the central region, showing hints of bluer colors, potentially suggesting some ongoing star formation, although at a low rate. The overall morphology is consistent with an elliptical galaxy, showing a slight deviation from perfect circularity. There may be signs of a minor gravitational disturbance, but it is not significant enough to suggest a major merger event.
