The galaxy presents as a concentrated elliptical morphology. The central region exhibits a high surface brightness, appearing nearly spherical with a smooth texture. A diffuse halo extends outwards, with a significant decrease in luminosity compared to the core. Color gradients are subtle but present, transitioning from a yellowish core to a slightly bluer outer region. No apparent spiral arms or dust lanes are visible. The overall structure suggests a relatively evolved system with a high degree of radial symmetry. The galaxy is neither experiencing a major merging event nor a strong merging disturbance.