The galaxy presents as a smooth, centrally concentrated object with a notably elliptical morphology. The primary color is a yellowish-orange hue, suggesting a population of older stars. There is some evidence of a smaller, bluer structure embedded near the core, indicating the potential presence of younger, hotter stars or an active galactic nucleus. Overall, the galaxy appears relatively undisturbed, but there may be an ongoing interaction with this bluer structure. The outer regions are fainter and blend gradually into the background sky.
