The galaxy presents as a centrally concentrated object with a generally smooth morphology. The shape is generally rounded but with some elongation, appearing more elliptical than perfectly circular. There are subtle irregularities or possible faint features, such as minor tidal disruptions, present in the outer regions, but the dominant impression is of a relatively undisturbed system. The overall appearance indicates that any interactions are either minor or occurred some time ago. The core is significantly brighter than the outer edges, suggesting a high density of stars or active galactic nuclei.
