The galaxy exhibits an elliptical morphology, appearing largely smooth with a high degree of central concentration. The light distribution suggests a well-defined spheroidal component, exhibiting a moderate ellipticity, appearing neither perfectly round nor highly elongated. There is faint evidence of a disk. The galaxy shows a color gradient, with a bluer hue in the outer regions transitioning to a yellower and redder hue in the central bulge, consistent with a population of older stars. No signs of strong tidal interactions or major disturbances can be discerned, although there is a faint irregularity in the outer halo.
