The galaxy presents as a relatively smooth, elliptical-like structure. It appears to have a bright central bulge that gradually diffuses into the outer regions. There is little evidence of spiral arms or distinct features, with no clear dust lanes visible. The light distribution suggests a fairly uniform stellar population. The galaxy exhibits a slight elongation, deviating from a perfectly circular shape. It displays a yellowish-white hue in the central region, possibly indicating a concentration of older stars, with a subtle shift towards bluer tones in the outer areas. Overall, the galaxy seems to be relatively undisturbed.
