The galaxy presents as a primarily smooth, elliptical structure with a bright central bulge dominating its overall appearance. The light distribution appears concentrated towards the center. The ellipticity is relatively low, appearing nearly circular. A faint disk-like structure might be present, or it might be an artifact from the imaging process. There are some indications of minor disturbances or asymmetries in the outer regions, but the overall structure appears relatively undisturbed. The color suggests a population of older stars, indicating a relatively low rate of star formation. There is a possible merging event occurring, with some minor disturbances evident. There is some faint blue light present in the outer parts of the galaxy, suggesting a bit of ongoing star formation.
