The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white glow, indicative of a high concentration of older stars, though a hint of green could indicate some areas of recent star formation. The galaxy appears relatively undisturbed, with no obvious signs of spiral arms or tidal features. The light intensity decreases gradually from the core outwards, with a slight elongation apparent in the outer regions. The overall color profile suggests a predominantly older stellar population.
