The galaxy presents as an elliptical morphology, characterized by a smooth, centrally concentrated light distribution. There is a subtle color gradient, transitioning from a bluer hue in the outer regions to a redder core. No distinct spiral arm structures or prominent dust lanes are discernible, suggesting a lack of active star formation in the primary body. The shape is slightly elongated. There is no evidence of a major merger event, however, there is a slight disturbance to the smooth shape which could potentially be an indication of a minor merger in the past.