The galaxy presents a generally smooth and homogenous appearance. It exhibits an elliptical morphology, appearing somewhat elongated in shape. The light distribution suggests a concentrated central region with a gradual decrease in luminosity towards the outer edges. No distinct spiral arms or prominent dust lanes are visible. The overall color is moderately red, indicative of an older stellar population and suppressed star formation. There is no obvious indication of any major ongoing merger activity or significant tidal disturbances. Faint asymmetrical features, probably small distortions, are seen.
