The galaxy presents as a fairly smooth, elliptical-like object, exhibiting a high degree of central concentration. Its color profile suggests the presence of an older stellar population, with a yellowish to reddish hue dominating its overall appearance. There is no discernible spiral arm structure or distinct dust lane visible. The galaxy appears largely undisturbed, showing no clear signs of ongoing major merger activity or significant tidal distortions in its morphology. It displays a compact profile. Faint color variations are observed within the galaxy, but they do not suggest recent intense star formation. The system is relatively isolated.
