The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal. It exhibits a concentrated central bulge, which displays a yellowish-orange hue, indicative of an older stellar population. The light gradually fades towards the outer regions, displaying a more reddish tint in the extreme outer edges, also suggesting an older, cooler stellar population. There are no apparent spiral arm structures or dust lanes visible. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal interactions. It possesses a high degree of roundness. There is no active star formation visibly occurring.
