The galaxy presents a somewhat diffuse morphology, appearing largely smooth and elliptical in shape, though with some subtle irregularities hinting at possible features or a disk-like structure. It exhibits a pronounced central bulge that gradually fades into a less luminous halo.

The galaxy's color profile suggests a mixed stellar population. The central bulge shows a yellowish hue indicative of older, redder stars, whereas the outer regions present a slightly bluer tint, implying the presence of younger, hotter stars and ongoing star formation. There are no readily apparent spiral arms or distinct dust lanes visible. Overall, the galaxy appears relatively undisturbed, showing no major signs of ongoing mergers.
