The galaxy presents a largely smooth, rounded morphology. There is little indication of spiral arm structure or significant disk features. The light distribution is generally centrally concentrated, with a gradual decrease in intensity moving outwards from the core. The galaxy's color appears yellowish-orange, suggesting an older stellar population, possibly dominated by evolved stars. There is no obvious active galactic nucleus, or dust lane. The overall impression is of an elliptical-type galaxy at an intermediate distance, with a relatively high degree of sphericity. There are no obvious signs of recent or ongoing major mergers, though there might be some indication of a minor disturbance in its structure.
