The galaxy presents as a relatively small, disk-dominated spiral galaxy, viewed at an oblique angle, but not quite edge-on. The disk exhibits noticeable spiral arm structure, although the arms are not sharply defined, appearing somewhat flocculent. Star formation is evident within these arms, indicated by the presence of bluer regions. A central bulge is discernible, but it appears relatively small compared to the overall disk size. There is no immediately obvious strong bar feature. The morphology of the galaxy suggests that it is in a relatively quiescent state.
