The galaxy presents a generally smooth morphology. Its central region exhibits a concentrated, bright luminosity that fades outwards. The color gradient transitions from a yellowish-white core to an outer halo with faint blue hues. The overall shape approximates a sphere, showing minimal signs of disk-like structures or distortions indicative of recent major merging activity. Subtle irregularities are observed in the outer halo, possibly indicating minor disturbances. The galaxy appears as a single, relatively undisturbed object, its light indicative of a stellar population with a mix of ages. Star formation is evident though at a low rate, possibly localized in the outer regions where blue hues are visible.
