The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, centrally concentrated light profile. There is little evidence of spiral arm structures or significant dust lanes. The galaxy appears largely spheroidal in shape, displaying a high degree of central symmetry with a slight elongation. Its color index suggests a population of older stars, with a yellowish-orange hue dominant, indicative of evolved stellar populations. The galaxy shows no obvious signs of recent or ongoing major merger activity or tidal disturbances in this image, suggesting it is a relatively undisturbed system. There appear to be no very blue, young stars or star forming regions visible. The light is generally evenly distributed with the most intense luminosity coming from the center. 