The galaxy presents as a centrally concentrated, luminous object with a largely smooth morphology. Its overall shape appears elliptical and generally round. There is a hint of a slight deviation from perfect circularity, but it is subtle. The galaxy lacks any obvious spiral arm structures or dust lanes. There are no prominent tidal features, plumes, or distortions suggestive of a recent major merger event, though there appears to be a minor disturbance, maybe in the form of a faint, extended halo. The galaxy exhibits a radial color gradient, appearing bluer in the outer regions and redder towards the center, indicating a possible difference in stellar populations or dust content between these areas.
