The galaxy presents a primarily smooth, elliptical morphology. Its core exhibits a concentrated, bright yellow hue, gradually diffusing outward into a fainter halo. The isophotes appear elongated, with a moderate ellipticity. Hints of faint, extended structures are visible, although poorly defined against the background sky. No distinct spiral arms or prominent dust lanes are discernible. The overall color suggests a relatively old stellar population, indicative of a mature system with suppressed star formation. Minor asymmetry on the right side of the halo may imply a recent interaction or merger event.
