The galaxy appears to be a spiral type, viewed at a significant angle. The central bulge is not particularly pronounced. There seems to be some unevenness, or perhaps a minor disturbance visible in the spiral arms. The arms themselves are not tightly wound, exhibiting a more open structure. There may be evidence of an ongoing minor merger or interaction, indicated by subtle distortions in the galactic disk. A very low level of star formation may be present.
