The galaxy presents as a smooth, centrally concentrated object. Its morphology is largely elliptical, appearing approximately circular on the plane of observation, with a slight hint of elongation. The core exhibits a bright, yellowish-white hue that dominates the galaxy's luminosity profile. Proceeding outwards, the galaxy transitions into a green tinged, diffuse halo. There is no discernable spiral arm structure. The light distribution suggests minimal dust obscuration, and the overall structure appears undisturbed, indicating little recent interaction or merger activity. Based on the color and morphology, the galaxy likely consists of a relatively old stellar population, with little ongoing star formation.
