The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct substructures. There is a slight elongation, suggesting it is not perfectly spherical but rather closer to an intermediate elliptical shape. Color gradients are subtle; the central region appears slightly yellowish-white, indicating the presence of older stellar populations, while the outer regions exhibit a fainter, bluer hue, perhaps hinting at a low level of ongoing star formation. No signs of strong tidal interactions or major disturbances are evident in its morphology.
