The galaxy presents an elliptical morphology. The light distribution appears relatively smooth and centrally concentrated, with a moderate color gradient from the center outwards. There is evidence of a possible interaction or merger event, displayed by an elongation in its shape. There is some faint blue light. A significant portion of the light comes from older stellar populations. The galaxy's overall appearance suggests it is in an advanced stage of evolution, possibly undergoing a transition towards a more quiescent state with a suppressed star formation rate.
