The galaxy presents as a luminous, centrally concentrated object. Its overall form is ellipsoidal. The central region exhibits a bright, yellowish-white hue, suggesting a substantial population of older stars. Moving outward from the core, the light gradually diminishes, transitioning into a more diffuse halo. There is a subtle asymmetry in the outer regions, but no strong indication of spiral arm structure or significant dust lanes within the galaxy itself. The smooth appearance suggests a relatively quiescent system, potentially an elliptical galaxy undergoing limited star formation.
