The galaxy appears to be a spiral galaxy, viewed at an oblique angle to our line of sight. There is an indication of spiral arm structure, with several arms visible. These arms appear somewhat tightly wound. The galaxy exhibits a noticeable central bulge region. Within the disk, there are regions of intense star formation which can be seen as bright blue. The galaxy does not show any obvious signs of a major disturbance, such as tidal tails or strong asymmetries, but is slightly elongated along one axis. Based on the diffuse light distribution, the galaxy has a relatively smooth light profile.
