The galaxy appears to be a spiral galaxy viewed at a significant angle, but not quite edge-on. The disk is prominent, showing hints of spiral arm structure; these arms are somewhat flocculent. There appears to be a central bar feature contributing to the galaxy's overall structure. The bulge is of moderate size relative to the disk. Based on color indices the star formation rate appears low. There are indications of some minor tidal disturbances or interactions with another nearby galaxy, but it is ambiguous.
