The galaxy presents as a fairly smooth, elliptical or lenticular object. There is a concentrated central bulge with a gradual fading of luminosity towards the outer regions. The core exhibits a warmer, reddish-orange hue, possibly indicating an older stellar population. The surrounding regions appear slightly bluer, suggesting the presence of some younger stars or ongoing, albeit limited, star formation. There are no apparent spiral arm structures or prominent dust lanes visible. The overall shape suggests a system that is relatively undisturbed, showing no strong signs of recent or ongoing merger activity.
