The galaxy presents as a centrally concentrated, ellipsoidal structure. The core exhibits a high degree of luminosity, appearing nearly uniform and intensely bright with a yellowish hue, suggestive of an older stellar population. Fainter, more diffuse, extensions emanate outward from the central bulge, exhibiting a smoother texture. A subtle flattening can be observed. Evidence of a distinct disk component or spiral arms is not readily apparent in the image, nor are any signs of irregular morphology or recent major merger events. Overall, the system's light distribution supports a classification towards an early-type galaxy with a significant spheroidal component and little ongoing star formation activity.
