The galaxy presents as a centrally concentrated, elliptical-like system. Its morphology appears generally smooth, lacking prominent spiral arms or distinct features. The color profile indicates a dominant population of older stars, visible in the yellowish-red hue of the core. There might be some evidence of a small amount of ongoing star formation, indicated by the very faint green in the galaxy's center. Overall, the galaxy seems relatively undisturbed, exhibiting no strong signs of recent major merger activity. Its apparent size is compact.
