The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high degree of luminosity, appearing nearly spherical and concentrated. Proceeding outwards from the core, the luminosity gradually diminishes. There are very minimal visible features, with a distinct lack of prominent spiral arms or other major structural disturbances. The galaxy appears to be relatively isolated, showing no clear signs of ongoing or recent major mergers or tidal interactions. The overall color profile suggests a population of older stars, as indicated by the reddish hue. The lack of blue light suggests a relatively low star formation rate.
