The galaxy presents as a relatively smooth, centrally concentrated light distribution. There is minimal discernible substructure, lacking spiral arms or a prominent bar. The central region exhibits a brighter, slightly more compact core, suggesting the presence of a galactic bulge. The overall shape appears roughly circular, deviating little from a perfect ellipse. There are no obvious signs of tidal tails, shells, or other features indicative of recent major mergers, though some minor irregularity in the outer isophotes hints at a possible past interaction. The color profile displays a gradual transition from a slightly bluer hue in the outer regions to a redder hue in the central bulge.
