The galaxy presents as a spiral type. A central bulge is visible, though it appears relatively indistinct, transitioning smoothly into the surrounding disk. The spiral arms are well-defined, winding moderately tightly around the bulge, though somewhat ill defined in the outer edges of the galaxy. These arms are traceable, with possibly two dominant arms. The galaxy's disk exhibits a noticeable blueness suggesting ongoing star formation. No obvious bar structure is apparent. There is some indication of a minor disturbance in the galaxy's morphology, with a small asymmetry in the disk, though it does not appear to be undergoing a major merger event. The galaxy disk is more face-on than edge on, as indicated by the clear visibility of the spiral arms.