The galaxy appears to be a spiral galaxy with a prominent disk. The spiral arms are well-defined and exhibit a blue hue, indicating recent star formation. The bulge is relatively small, contributing only moderately to the overall luminosity. There is no obvious central bar structure visible, but a weak presence cannot be ruled out. The galaxy is viewed at an angle, not quite face-on, but also not edge-on. There may be some minor tidal disturbances, suggesting possible interactions or past mergers, but no major merging events are readily apparent. The disk component exhibits more features than the bulge. 
