The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated bulge that appears yellowish-white, suggesting an older stellar population in the core. The galaxy's light profile decreases gradually from the center outward, showing no prominent spiral arms or distinct features. There may be a faint disk component as indicated by the slight elongation and more blue hues on the periphery. Overall, it seems to be a well-defined, relatively undisturbed galaxy.
