The galaxy appears as a centrally concentrated, elliptical-like structure. Its core region exhibits a bright, yellowish hue, suggesting a population of older stars. This central region transitions smoothly outwards, displaying a gradual decrease in luminosity. The outer regions show a faint greenish color. There is no apparent spiral arm structure or significant dust lane obscuration visible. The galaxy's overall form appears relatively undisturbed, with no major signs of tidal disruption or ongoing merger activity apparent in this image. 
