The galaxy appears to be a luminous, elliptical system exhibiting a smooth morphology with a dominant, centrally concentrated bulge. There may be some signs of a past interaction, but the galaxy appears mostly undisturbed. The light profile suggests an older stellar population, with a redder color index. The system is relatively compact and massive, which is consistent with a low rate of star formation. Although the classification is not fully defined, there may be some characteristics of a merger. 
