The galaxy presents as a somewhat elliptical object with a bright, concentrated central bulge. Its light distribution appears relatively smooth overall, though there are hints of asymmetry or faint disurbance in the outer regions, possibly indicating tidal interactions or recent minor mergers. The color gradient suggests an older stellar population dominating the central bulge, with bluer tones present in the outer regions hinting at more recent star formation. There is a notable lack of prominent spiral arm structure. The overall morphology appears somewhere between elliptical and lenticular.
