The galaxy presents as a centrally concentrated, predominantly smooth, elliptical-like structure. Its core is a bright, yellowish-white, indicating a population of older stars. The intensity of the light decreases gradually from the center outwards, suggesting a relatively even distribution of stars.

There is a slight extension to one side, which may imply minor tidal interaction or a faint disk-like structure. Overall, the galaxy appears relatively undisturbed with little to no evidence of major star formation regions or significant dust lanes, consistent with a more evolved system. The galaxy possesses an apparent reddish hue which suggests a degree of star formation activity.
