The galaxy presents as a relatively smooth, elliptical morphology. Its color is predominantly yellow-orange, suggesting an older stellar population with minimal ongoing star formation. The light distribution appears concentrated towards the center, with a gradual decrease in intensity towards the outer regions. No distinct spiral arms or disk-like structures are visible. The overall structure indicates a system that is likely spheroidal in shape. There are no obvious signs of tidal disturbances or mergers, implying a relatively isolated evolutionary history.
