The galaxy presents a distinct disk-like morphology, viewed at an angle slightly offset from face-on. The central bulge is prominent and appears relatively bright and concentrated. A strong bar structure is clearly visible, bisecting the bulge and extending outwards into the disk. The spiral arms are present, albeit somewhat diffuse and not tightly wound. There are several distinct regions of star formation within the disk. The galaxy does not appear to be undergoing a major merger, but some degree of minor disturbance or interaction cannot be ruled out. Overall, the galaxy appears to be a barred spiral with ongoing, but relatively low, star formation activity.
