The galaxy presents as a moderately bright object with an elliptical morphology. Its core region appears luminous and concentrated. The galaxy exhibits a smooth overall appearance with a gradual decrease in light intensity moving outward from its center. There is a hint of a possible disk-like feature or ring structure with possible emission lines. This feature is oriented approximately horizontally. There is the possibility of minor tidal disturbances, or a recent merger event evidenced by some irregularities in the outer regions.
