The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a pronounced concentration of light, appearing nearly circular. The light distribution transitions smoothly from the bright central region outwards, with no apparent spiral arm structures or significant dust lanes visible. There's a subtle color gradient noticeable, with the core exhibiting a slightly redder hue compared to the fainter outer regions, which appear more greenish-white. This color difference may indicate a difference in stellar populations, where the core is dominated by older, redder stars while the outer regions contain more younger, bluer stars, although star formation seems subdued. The overall symmetry suggests a relaxed dynamical state, with no obvious signs of recent major mergers or significant tidal disturbances. The galaxy appears largely undisturbed, representing a relatively evolved system.
