The galaxy presents as a smooth, elliptical morphology, with a high degree of central concentration. The light profile appears to be relatively uniform, lacking prominent spiral arms or distinct features. There is a slight elongation. The color index suggests an older stellar population, dominated by redder wavelengths, with minimal evidence of ongoing or recent star formation. The overall appearance is consistent with a massive galaxy that has largely exhausted its supply of gas and dust, or that may have minimal star formation in general. There's no visual evidence of major mergers or significant tidal disturbances.
