The galaxy presents as a concentrated, elliptical morphology. Its core exhibits a bright, yellowish-orange hue, indicative of an older stellar population. The light appears to gradually fade towards its outer edges. There is no visible spiral structure or distinct dust lanes. The overall form is largely smooth and undisturbed, with no apparent signs of ongoing major mergers or tidal disruptions. The galaxy is neither perfectly round nor significantly elongated, showing an intermediate ellipticity.
