The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. Its color gradient transitions from a yellowish-white core to a subtly bluer halo, indicating potential variations in stellar populations. No distinct spiral arm structures or dust lanes are discernible. The shape of the galaxy appears nearly circular. There is no evidence of any major mergers or tidal disturbances within the system. The estimated mass of the galaxy is likely significant, although it exhibits relatively low star formation activity.
