The galaxy presents a generally elliptical morphology, appearing largely smooth and centrally concentrated. It exhibits a bright, relatively large core that gradually fades into an extended halo. The light distribution suggests a relatively old stellar population, with a color gradient transitioning from a yellowish core to a slightly bluer outer region. There is little evidence of prominent spiral arm structure or significant dust lanes. The overall appearance suggests an evolved system, potentially undergoing relatively little active star formation at the present epoch. Some minor asymmetry in the outer halo luminosity is apparent. Based on the shape, it could either be a round elliptical galaxy or a lenticular galaxy that is viewed primarily face-on. There is not much evidence of any major mergers or distortions.
