The galaxy presents as an elliptical morphology, appearing largely smooth and featureless. There is a concentrated central bulge of moderate luminosity, surrounded by a more diffuse halo. The radial color gradient suggests a population of older stars within the central region, exhibiting a yellowish-orange hue. Moving outwards, the halo appears subtly bluer, potentially indicating the presence of a younger stellar population or a small amount of ongoing star formation. The galaxy shows a slight elongation, hinting towards a shape that is not perfectly spherical. No distinct spiral arms or dust lanes are observed. The galaxy appears relatively undisturbed, lacking any obvious signs of recent mergers or tidal interactions.
