The galaxy presents as a spiral structure with two prominent arms, although several fragmented arm segments also appear. The overall winding of the spiral arms appears to be of medium tightness. A central bulge is observed, and it appears relatively small in relation to the disk. The galaxy has an inclination that is moderately face-on, allowing the spiral structure to be clearly visible. There is a hint of a bar-like structure, but it is very weak. The disk component exhibits a mottled texture, and the color is dominantly blueish. There are no immediately obvious signs of major merger events, although some features are consistent with a minor disturbance in the galaxy.