The galaxy appears to be a spiral type, viewed at an oblique angle. Evidence of spiral arms is visible, although the structure is somewhat flocculent and not sharply defined. A prominent central bulge is not apparent; instead, the brightness of the galaxy gradually increases towards a central region. The arms are populated with what appear to be star-forming regions, indicated by the presence of blue-ish knots. The overall color of the galaxy indicates a mix of stellar populations, with both younger, bluer stars and older, redder stars present. There are no obvious signs of a major ongoing merger, though there might be some tidal features present as minor disturbances. The galaxy's disk appears to be relatively thick, and the bar structure is not very distinct.