The galaxy presents a generally smooth, elliptical morphology. Its overall color profile indicates a greater abundance of older stellar populations, suggesting a relatively low star formation rate. There is little evidence of spiral arms or significant dust lanes. The galaxy exhibits a high degree of central concentration, with light intensity decreasing gradually towards its outer edges. There are no signs of ongoing major mergers or tidal disturbances, although very subtle minor irregularities cannot be completely ruled out. The galaxy's shape is approximately round.
