The galaxy presents a distinct spiral morphology. It is observed at a near face-on orientation, revealing prominent, loosely wound spiral arms. These arms exhibit a blue hue indicative of active star formation, interspersed with regions of older stellar populations, exhibiting a yellow-red color. A central bulge is discernible, with an intermediate size. No strong bar structure is immediately evident. There are signs of a possible ongoing or recent merger event due to some morphological disturbances, which could explain the loose and extended spiral arms.
