The galaxy presents as a relatively small, edge-on disk galaxy. Its appearance is largely smooth, suggesting a relatively homogenous stellar population. The central bulge region appears prominent and moderately concentrated. Its shape is somewhat rounded rather than boxy. The overall color of the galaxy is slightly reddish, which could indicate an older stellar population and/or the presence of dust. While there appears to be no strong spiral arm structure visible, the faintness of the outer regions of the disk suggests that it is relatively undisturbed. There are no other galaxies near enough to assume there is a merger occurring, although there is a slight asymmetrical appearance in the outer regions.
