The galaxy presents as a spiral structure, exhibiting a noticeable central bulge. The spiral arms appear prominent and well-defined. The winding of the spiral arms appears to be tightly wound. There is evidence of active star formation within the arms, indicated by their bluish hue. Overall the galaxy does not appear smooth and seems to exhibit a featured and disc-like morphology. There appears to be a bar within the galaxy. The galaxy is undisturbed and is not experiencing a major merger. 
