The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a largely elliptical morphology, appearing quite round in projection. There is a lack of any discernible spiral arm structure or distinct features suggestive of active star formation regions. The light distribution suggests that it is dominated by older stellar populations, which are likely responsible for the redder color. There are no obvious signs of recent or ongoing major mergers or tidal disturbances. Given its estimated distance, this galaxy can be classified as quite massive.
