The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a yellowish-orange hue, indicative of an older stellar population. The radial color profile suggests a moderate color gradient, with bluer regions observable towards the periphery, possibly signaling ongoing star formation. There is a small hint of a disk. The overall shape is somewhat rounded, deviating slightly from a perfect sphere. There is an indication of a minor disturbance, which may be caused by interaction or internal effects.
