The galaxy appears as a centrally concentrated object. The core region exhibits a bright, intense luminosity, potentially indicative of an active galactic nucleus or a region of intense star formation.

Surrounding the core, a less intense, bluer halo is visible. The halo appears relatively smooth and featureless with a slight oblong shape. There is a subtle color gradient moving outwards from the center.

The overall morphology suggests a relatively undisturbed system, lacking any prominent spiral arms or significant tidal features, or any signs of major mergers, though faint asymmetric features are present.

The presence of the blue halo suggests ongoing star formation, contrasting with the potentially older stellar population concentrated in the core.
