The galaxy presents as a primarily smooth, centrally concentrated object. It exhibits a moderate ellipticity, appearing more 'in between' round and cigar shaped rather than perfectly circular. The central region displays a yellowish hue, potentially indicative of an older stellar population. Surrounding the core is a broader, somewhat fainter region showing hints of greenish color, which might suggest the presence of some younger stars or ongoing star formation, although at a relatively low rate. There is no strong evidence of major mergers or significant tidal disturbances in the immediate vicinity, though some subtle asymmetries or minor disturbances cannot be entirely ruled out. Overall, the galaxy seems to be an intermediate system, exhibiting characteristics of both smooth elliptical galaxies and those with some degree of ongoing activity.
