The galaxy presents a generally smooth and rounded morphology. It appears elliptical in shape, lacking any prominent spiral arm structure or a well-defined disk. The light distribution is centrally concentrated, with a bright core that gradually fades outwards. The color gradient suggests a population of older stars dominating the galaxy's composition, with a yellowish-red hue characteristic of evolved stellar populations. There are no obvious signs of active star formation regions or significant dust lanes. The overall impression is that of a mature, relatively quiescent galaxy. There is perhaps a slight indication of a minor asymmetry or disturbance in the outer regions, but it is not conclusive enough to suggest a recent major merger event. The galaxy seems to be relatively isolated and undisturbed.
