The galaxy presents a predominantly smooth and rounded morphology. It exhibits a concentrated central bulge with a gradual decrease in surface brightness towards the outer regions, suggesting an elliptical or lenticular classification. No spiral arms, dust lanes, or distinct features are readily apparent. The galaxy's color index suggests an evolved stellar population and low current star formation activity. There is no visual evidence of tidal disturbances or ongoing mergers; the overall structure appears relatively undisturbed.
