The galaxy presents a largely smooth and elliptical morphology. There is little to no evidence of spiral arm structure or significant dust lanes. The central region exhibits a bright, concentrated bulge, suggesting a relatively high stellar density. The color gradient transitions smoothly from a yellowish-white core to a slightly bluer, fainter halo or outer envelope. The overall rounded appearance indicates a low degree of rotational support, consistent with an early-type galaxy classification. There are no visually apparent signs of ongoing major mergers or significant tidal disturbances. Minor irregularities may exist but are not readily discernible at this resolution.
