The galaxy appears to be an elliptical type, exhibiting a generally smooth and rounded morphology. The light is concentrated towards the center, with a gradual decrease in intensity extending outwards. The galaxy appears relatively undisturbed, showing no major signs of tidal interactions or ongoing mergers. The galaxy displays a subtle color gradient, appearing bluer towards the outer edges and redder in the core, which may suggest differing stellar populations. There is little evidence of spiral arm structure or dust lanes.
