The galaxy presents as a single, centrally concentrated object with a smooth, largely featureless morphology. The light profile appears nearly symmetrical, with a gradual decrease in intensity from the core outwards. The galaxy exhibits a color gradient, shifting from a yellowish-white hue at the core to a redder tone at the periphery. No spiral arm structures or distinct dust lanes are discernible within the limitations of the available image resolution. The overall shape is somewhere between round and elliptical. There is no strong evidence of significant ongoing mergers or major tidal disturbances. The galaxy appears relatively undisturbed.
