The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. There is a subtle color gradient visible, transitioning from a yellowish-white core to a slightly bluer outer halo. The galaxy exhibits a relatively high degree of roundness, with only a slight deviation from a perfect circular shape. No distinct spiral arm structures or significant dust lane obscuration is apparent. There may be some evidence of minor disturbances in the morphology, but they are not prominent. The object appears to be a relatively evolved system, potentially with a significant population of older stars.
