The galaxy presents a largely smooth and rounded morphology. The core exhibits a concentrated, bright yellowish-white luminosity, potentially indicating an older stellar population. The outer regions display a more diffuse halo of light, gradually fading into the background sky. There is a slight reddish tinge visible in certain areas, which might suggest the presence of dust or regions of ongoing, albeit subdued, star formation. No prominent spiral arms or other distinct features such as bars or tidal tails are readily apparent. The overall structure appears relatively undisturbed, exhibiting no clear signs of recent major merger events. The galaxy presents a structure consistent with that of an elliptical galaxy.
