The galaxy presents as a generally smooth and centrally concentrated object. The light distribution suggests an elliptical morphology, or potentially a lenticular galaxy seen at a sufficient distance that obscures any disk structure. The core of the galaxy exhibits a bright, yellowish hue, indicative of an older stellar population likely dominated by red giant stars. Proceeding outwards from the core, the color transitions to a bluer hue, implying the presence of a younger, hotter stellar population in the outer regions, although the overall blue fraction is relatively low. There's no clear evidence of spiral arms or significant dust lanes. Faint features around the galaxy suggests a lack of major disturbances or ongoing mergers. The galaxy appears relatively isolated.
