The galaxy appears to be a spiral galaxy viewed at a significant angle, perhaps close to edge-on. There is evidence of a central bulge, though it is not very prominent. Faint arms can be discerned with moderate disturbance within the galaxy. The arms appear clumpy, likely due to active star formation regions. Light from the galaxy is dominant in the redder wavelengths, with a weak detection in the bluer bands. There is a suggestion of a possible minor merger or tidal disturbance impacting the shape and structure of the galaxy.
