This galaxy presents a morphology consistent with a spiral structure, viewed at an angle somewhere between face-on and inclined. Prominent spiral arms are observed, exhibiting a flocculent pattern. The arms appear loosely wound. The central bulge of the galaxy is noticeable, of moderate size. Evidence suggests the presence of a bar-like structure within the central region, but it is difficult to say with certainty. The galaxy displays a blue hue, potentially indicative of active star formation within the spiral arms. The disk appears somewhat disturbed, possibly due to a minor interaction or internal processes.
