The galaxy presents as a spiral structure, oriented approximately face-on relative to our line of sight. A central bulge region is evident, appearing moderately compact, and a relatively small size when compared to the galactic disc. This appears to be a barred spiral galaxy. Two distinct spiral arms emanate from the ends of the galactic bar. These arms wind tightly around the central bulge, before becoming patchy and less distinct as they reach the edge of the galaxy. Some diffuse, blue-ish star forming regions are suggested in the arms, however they are not particularly well defined. There is no indication of any significant ongoing merger activity or major morphological disturbance.
