The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The galaxy's color is predominantly yellowish-orange, suggesting an older stellar population with lower rates of recent star formation. No distinct spiral arm structures or dust lanes are readily apparent. There is very little indication of any tidal disturbances or ongoing mergers. Its overall morphology points to a relatively undisturbed system, with no significant indications of active galactic nuclei (AGN) activity.
