The galaxy presents a largely smooth, elliptical morphology with no discernible spiral arm structure. The light distribution is centrally concentrated, with a gradual decrease in surface brightness moving outwards from the core. The galaxy exhibits a subtle color gradient, shifting from a yellowish-white core to a slightly bluer, less intense halo. The overall form appears largely undisturbed, with no major asymmetries or tidal features suggesting recent major merger activity. There may be some minor irregularities or faint extensions hinting at potential low-level interactions, but further analysis is needed to confirm.
