The galaxy presents a somewhat rounded morphology. A central, bright region dominates the structure, with a noticeable radial decrease in surface brightness outwards. The core exhibits a blue-green hue, suggestive of possible recent star formation activity. The outer regions display a more yellow-red color profile. There is evidence of morphological disturbance in the structure. The outer edges of the galaxy appear irregular, hinting at possible tidal interactions or ongoing merger activity. The galaxy is not perfectly smooth in appearance. The presence of subtle variations in color and luminosity across the structure implies underlying complexities, perhaps due to dust lanes or unresolved stellar populations.
