The galaxy presents as a spiral with a moderate inclination to our line of sight. Two spiral arms are clearly visible, and are wound at a medium tightness. There is a suggestion of multiple additional arms. A bar structure is visible traversing across the bright central bulge. The bulge component is of medium size, occupying a substantial portion of the central region. Star formation is evident in the spiral arms, showing as bluer and more diffuse. There is no obvious ongoing merging activity.
