The galaxy presents as a spiral type, with a disk-like morphology. Two distinct spiral arms are discernible, though the structure exhibits a somewhat flocculent nature. A bar feature appears to be present, with moderate prominence, bisecting the central region. The bulge is somewhat contained. The spiral arms exhibit a medium degree of winding, extending outwards from the central bulge. There is no apparent major merger or significant disturbance in the overall structure. The galaxy's light profile suggests ongoing star formation, with a blue hue evident.
