The galaxy presents as a relatively smooth, elliptical morphology with a discernible central bulge. The color gradient suggests an older stellar population, with a yellowish-orange core gradually transitioning to a bluer halo. The elliptical shape indicates minimal rotational support and suggests the galaxy is likely the result of past mergers. There is little evidence of significant dust lanes or active star formation regions. The overall appearance is consistent with a passively evolving galaxy. The object exhibits an apparent cigar shape. There are no signs of any significant tidal disruption or ongoing merger activity within the visible structure. 
