The galaxy presents as a slightly inclined spiral galaxy. It exhibits loosely defined spiral arms, with regions of enhanced star formation that appear as subtle blue knots embedded within the arms. The central bulge region appears moderate in size and possesses a smooth texture. The overall color suggests an intermediate age stellar population, possibly transitioning from active star formation to a more quiescent state. There is no sign of a large disturbance in the galaxy, it looks relatively stable and non-interacting. Based on these features, the galaxy can be classified as an intermediate spiral, neither a grand-design nor a flocculent spiral.
