The galaxy appears as a centrally concentrated, relatively smooth object with a slightly elliptical morphology. The light distribution is brightest in the core, fading gradually outwards with no apparent spiral arm structures or significant dust lanes. There is a subtle color gradient from a slightly bluer periphery to a redder core. Based on its apparent smoothness, the galaxy may be an elliptical galaxy or a lenticular galaxy seen face-on. A lack of distinct features suggests it is not undergoing a major merger, however some minor disturbances cannot be ruled out from this image alone. Overall the galaxy presents as a mature system with limited ongoing star formation. 
