The galaxy presents a generally smooth, elliptical morphology. Its light profile appears centrally concentrated, with a diffuse halo extending outwards. There is some indication of a subtle disk-like structure. While the galaxy appears largely undisturbed, some asymmetries could point to minor interactions or internal processes. The colour profile suggests a relatively evolved stellar population, with a somewhat redder hue. There is the possibility of low-level star formation, as hinted by the bluish tint.
