The galaxy presents as a centrally concentrated, roughly circular object with a smooth appearance. Its core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The intensity gradually decreases outward from the core. There is a subtle gradient in color with the outer regions appearing slightly redder, potentially indicating a larger proportion of cooler, redder stars or dust obscuration in these areas. No distinct spiral arms or bar features are discernible; the light is rather diffuse. Overall, the galaxy appears relatively undisturbed.
