The galaxy presents a largely smooth, elliptical morphology. The central region displays a concentrated, bright core, suggesting a higher density of stellar population. The overall color gradient transitions from a yellowish-white core to a slightly redder, less luminous outer region, indicative of an aging stellar population. There is no apparent presence of spiral arms or distinct dust lanes. Faint extensions or tidal features cannot be ruled out, however, a recent or ongoing major merger event appears unlikely. The galaxy exhibits a relatively round shape, deviating only slightly from a perfect sphere.
