The galaxy presents as an elliptical morphology, appearing largely smooth in structure. The light distribution is centrally concentrated, with a bright, reddish core. The outer regions exhibit a gradual decline in brightness, transitioning to a greenish hue. There is a slight elongation along one axis, suggesting a deviation from perfect circularity, but the galaxy maintains an overall rounded appearance. No obvious spiral arms or significant dust lanes are visible. There are no clear indications of a recent or ongoing major merger event. Minor disturbances cannot be ruled out.
