The galaxy presents a smooth and centrally concentrated morphology, indicative of an elliptical or lenticular type. The light distribution appears relatively uniform across the visible extent, lacking prominent spiral arms or distinct features associated with active star formation. The core exhibits a bright, somewhat diffuse luminosity profile, suggesting a concentration of older stellar populations. The galaxy displays a generally rounded shape, though with a slight ellipticity. There's a subtle hint of disturbance or asymmetry in the outer regions, possibly indicating past interactions or minor gravitational perturbations. The color gradient appears to be consistent with an aging stellar population, trending towards redder hues.
