The galaxy presents as an elliptical morphology, exhibiting a smooth and diffuse light distribution. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The light profile suggests a somewhat spherical shape, though with a slight elongation. There appears to be a smooth radial gradient, with the central regions being brighter and redder than the outer regions, indicative of an aging stellar population towards the core. The galaxy's color suggests a lack of significant ongoing star formation.
