The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a generally elliptical morphology, showing a high degree of roundness. A prominent, bright core is observed, surrounded by a more diffuse halo. The color profile suggests a redder core transitioning to bluer outer regions, which could indicate a mix of older stellar populations in the center and younger stars in the outer disk. There's some subtle irregularity to the halo, hinting at possible minor disturbances or interactions. No distinct spiral arms or bar features are apparent in the visible light captured. Overall, the structure indicates a fairly massive galaxy with moderate levels of star formation.
