The galaxy presents a largely smooth morphology, appearing elliptical in shape. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer edges. The galaxy's color appears generally consistent throughout, with a slightly yellowish hue. There is no obvious evidence of spiral arms or significant dust lanes. The light distribution suggests a relatively old stellar population. The overall structure indicates a system that is likely dynamically relaxed, with minimal signs of recent mergers or tidal disturbances.
