The galaxy appears as a centrally concentrated object with a diffuse, extended halo. The core region exhibits a brighter luminosity, potentially indicative of a bulge component. The morphology appears largely smooth. There may be some mild asymmetries present in the outer regions, suggesting possible tidal disturbances or interaction with a smaller satellite galaxy. The galaxy is observed to be relatively blue, with a hint of redder color in the central regions. This suggests ongoing, or recent, star formation.
