The galaxy presents as a roughly elliptical structure, elongated along a northeast-southwest axis. It exhibits a smooth light distribution, lacking prominent spiral arms or a distinct central bulge. The color profile suggests a greater concentration of older stellar populations, indicated by the reddish hue. The lack of sharp features suggests a relatively evolved system, perhaps undergoing passive evolution. Faint tidal disturbances are visible, suggesting a past interaction with a nearby galaxy. The overall morphology leans towards a transition between elliptical and lenticular classification.
