The galaxy presents as a relatively smooth, elliptical object. It exhibits a concentrated central bulge, appearing nearly spheroidal in shape. The light profile suggests a system dominated by an older stellar population, with a redder hue towards the core transitioning to a slightly bluer tinge in the outer regions. There is a marginal indication of a faint, diffuse halo surrounding the main body of the galaxy, but the signal is weak. No apparent spiral arm structures or significant dust lanes are discernible within the visible portion of the galaxy. While the light is mostly smooth, there appear to be multiple points of high intensity suggesting the presence of either distinct galactic nuclei or potential areas of localized active galactic nuclei. There is no apparent tidal interaction or obvious morphological distortion implying major mergers, though the multiple potential nuclei does suggest that there could have been minor disturbances or interactions. 
