The galaxy presents as a relatively smooth, rounded structure. The light distribution suggests a centrally concentrated spheroid, lacking any discernible spiral arms or prominent disk features. The color appears yellowish-white, indicating a stellar population dominated by older, less massive stars. There is a faint, diffuse halo surrounding the central region, though its extent is difficult to ascertain. The galaxy shows no signs of major mergers or significant tidal disturbances, maintaining a relatively undisturbed morphology. It appears to be a quiescent system with a low rate of star formation, consistent with the observed color and lack of distinct features.
