The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually fades into the outer regions. The overall color appears to be moderately red-shifted, suggesting an older stellar population. There is little evidence of prominent spiral arms or significant dust lanes. A slight asymmetry can be observed in the outer regions, suggesting a possible past minor interaction or disturbance. The galaxy appears relatively isolated with no clear signs of ongoing merger activity.
