The galaxy presents a clear disk morphology, observed at an oblique angle, but not quite edge-on. Evident spiral arm structure extends from a central bulge. The spiral arms appear flocculent and well-defined, and exhibit a moderate winding. These arms contain regions of active star formation. A bar structure is present within the central region of the galaxy. The bulge appears small relative to the overall disk size. There is no obvious indication of a major ongoing merger, although there is subtle evidence of tidal disturbances or interactions with nearby objects.
