The galaxy presents as a relatively smooth, centrally concentrated object with a slight elongation. Its core region is noticeably brighter, exhibiting a yellowish-white hue that suggests an older stellar population. The outer regions display a fainter, bluer tint, possibly indicating regions of more recent star formation. There is no clear spiral arm structure visible, and the overall morphology points towards a galaxy that is more elliptical or lenticular in nature. No significant signs of tidal disturbances or ongoing mergers are readily apparent, which would otherwise show as irregular or extended features. The object is fairly symmetrical, with a gradual decrease in surface brightness from the core outward.
