The galaxy presents as a relatively smooth, elliptical structure. The light distribution appears concentrated towards the center, with a gradual decrease in intensity towards the outer regions. The galaxy is yellowish-white, suggesting an older stellar population. There is a slight elongation, but it could also be an indication of a minor tidal disturbance.

The system shows signs of a possible interaction or merger event. There may be signs of low-level star formation present. The overall structure indicates a significant mass.
