The galaxy presents a largely smooth, elliptical morphology, though not perfectly spherical. The overall color profile suggests a population of older stars, with a yellow-orange hue dominating the central region. There is a slight gradient outwards, with the outer regions showing a subtle shift towards bluer colors, hinting at the presence of younger, hotter stars in these areas, although star formation appears to be low. No distinct spiral arms or bar structures are discernible. The galaxy is relatively compact and well-defined, with a gradual decrease in luminosity from the core to the edges. There is no evidence of major mergers or significant tidal disturbances in the immediate vicinity. There is a possibility of minor disturbances or faint tidal tails, but the clarity of the image is not sufficient to confirm. The overall structure is consistent with an early-type galaxy, possibly undergoing passive evolution.
