The galaxy presents as an elliptical morphology, exhibiting a smooth, relatively featureless structure. The light profile suggests a centrally concentrated spheroid. The core is a bright yellowish-white, with a gradient in color temperature. A fainter bluish halo extends outwards, indicative of a stellar population that is slightly more active than the core. The overall symmetrical shape suggests a relaxed system, unperturbed by recent major mergers. There might be slight tidal interactions or minor disturbances evident, but overall the galaxy appears to be undergoing very little star formation throughout.