The galaxy presents as a spiral, viewed at an oblique angle. The disk is clearly visible, exhibiting a flocculent spiral structure. Two dominant spiral arms can be discerned extending from the central bulge. The spiral arms exhibit loose winding. The central bulge appears moderately sized and has a noticeable bar structure. Blue star formation regions are present within the spiral arms, especially near the outer edges of the disk, which indicates ongoing star formation. The galaxy exhibits some minor disturbances, which could be indicative of a recent or ongoing interaction or minor merger event. The central region appears more yellow/orange, suggestive of an older stellar population.
