The galaxy presents as a relatively smooth, elliptical-like structure. The primary body exhibits a centrally concentrated light profile, with a gradual decrease in luminosity towards the outer regions. The galaxy displays a yellowish-white hue, suggestive of an older stellar population. No prominent spiral arms or distinct dust lanes are discernible. There are no signs of any major disturbances or tidal features indicative of recent or ongoing mergers, though subtle asymmetries might be present upon closer inspection. The overall morphology appears generally regular and undisturbed.
