The galaxy has a short central bar, much like the Milky Way and very extended spiral arms.[4] The central disk appears to be rotating in the opposite direction to the extended spiral arms.[5]
The reason for the spiral arms and majority of the galaxy's disk to be still neutral hydrogen (as opposed to have formed stars) is not well understood but is thought to be related to the galaxy's isolation, in that it has no nearby satellite galaxies and no nearby major galaxies to force star formation.[4]
^"Archived copy". wwwatnf.atnf.csiro.au. Archived from the original on 12 July 2002. Retrieved 30 June 2022.{{cite web}}: CS1 maint: archived copy as title (link)