The galaxy presents as a compact, relatively small object. It exhibits a primarily smooth morphology, with some suggestion of internal structure. The dominant feature is a bright central region exhibiting a bluish hue, indicating the presence of hot, young stars or active galactic nucleus activity. There is a hint of a ring-like structure surrounding the central region. Overall, the galaxy does not present strong evidence of a disk-like structure, major mergers, or significant disturbances. 
