The galaxy presents as a largely smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing mostly round in shape, with a slight elongation along its major axis. The galaxy's core region displays a yellowish hue, suggestive of an older stellar population. The outer regions show a bluer color, which indicates the presence of some younger, hotter stars and potential ongoing, albeit low, star formation. There are hints of faint, diffuse features or a very faint disk extending outwards. The general symmetry and lack of significant distortions suggest that the galaxy is relatively undisturbed, showing no signs of a major merger event.
