The galaxy presents as a generally smooth, elliptical structure, exhibiting a concentrated central bulge that graduates outwards to a diffuse halo. The core region is notably bright, displaying a yellowish-white hue, suggesting a population of older stars. The outer regions show a slight elongation. A faint hint of structure is noted to the lower right with what appears to be a tidally disrupted area of fainter stars. The overall symmetry indicates a system that may be relatively relaxed, potentially nearing the end stages of a merger process, or a post-starburst system with low current star formation activity. The color gradient implies a relatively homogenous stellar population across the galaxy, with little evidence of young, blue stars in the outer regions.
