  We present the first visible wavelength images of the GG Tauri circumbinary
ring, obtained with the Hubble Space Telescope's Wide Field and Planetary
Camera 2. Scattered light from the ring is detected in both V and I band
images. The images show that the ring is smooth, except for a small gap that
could be a shadow caused by material between the stars and the ring. The spokes
seen extending from the stars to the ring in ground-based adaptive optics
images are not seen in our data, which suggests that they may be image
artifacts. The nearside/farside surface brightness ratio is 6.9 in I band,
consistent with forward scattering by small dust grains. The azimuth of the
peak ring surface brightness appears offset by 13 degrees from the azimuth
closest to us, as seen in previous near-IR HST observations. This may indicate
that the ring is warped or somehow shadowed by the circumstellar disks. The
color of the ring is redder than the combined light from the stars as observed
by HST, confirming previous measurements that indicate that circumstellar disks
may introduce extinction of light illuminating the ring. We detect a bright,
compact arc of material 0.3 arcseconds from the secondary star at an azimuth
opposite the primary. It appears to be too large to be a circumstellar disk and
is not at the expected location for dust trapped at a Lagrange point.
