The galaxy presents as a relatively compact and smooth object. It exhibits a generally elliptical morphology, appearing largely rounded in shape. There is no discernible spiral arm structure or significant disk component visible. The color profile indicates a redder central region transitioning to slightly bluer outer edges. This suggests the presence of an older stellar population concentrated towards the center, with a relatively lower ongoing star formation rate. There is no visible evidence of recent or ongoing major mergers or tidal disturbances affecting the galaxy's overall structure. It is a relatively massive galaxy, that has a estimated redshift suggesting that is receding away from us.
