The observed galaxy presents a distinct spiral morphology. The spiral arms are readily apparent, exhibiting a somewhat tightly wound structure. A central bulge is visible, but appears relatively small in proportion to the overall galactic disk. The galaxy's disk appears slightly inclined relative to our line of sight, but is not edge on. Evidence suggests a possible weak bar structure within the central region. The color of the arms indicates the presence of recent star formation. There is no indication of any major merging events.
