The galaxy presents a largely smooth and elliptical morphology. The central region exhibits a concentration of light, appearing yellowish-white, indicative of a population of older stars. A fainter, bluer halo surrounds the core, suggesting the presence of a younger stellar population and potentially some ongoing star formation. There is no apparent spiral structure or distinct dust lanes visible. The galaxy appears relatively undisturbed, with no obvious signs of a recent major merger event or tidal interactions. It has an estimated size of approximately 6 kiloparsecs.
