The galaxy appears to be an elliptical galaxy, characterized by a smooth, generally featureless morphology. Its shape is somewhat elongated, but predominantly round. The color profile indicates a higher concentration of older stellar populations, resulting in a yellowish to reddish hue. No significant dust lanes or spiral arm structures are discernible. There is no evidence of major ongoing mergers or tidal disturbances. A slight asymmetry may indicate a minor interaction in the past. The galaxy appears relatively isolated.
