  We present VLA maps of the Seyfert 2 galaxy NGC 7319 at 3.6, 6, and 20 cm.
Sub-arcsecond resolution is achieved at 3.6 and 6 cm. The radio emission
exhibits a triple structure on a scale of ~4'' (1.7 kpc). All three components
have steep spectra, consistent with synchrotron radiation. We have also
analyzed an HST archival, broad-band red image, which contains structure
related to the radio components. In particular, a V-shaped feature in the HST
image some 3.7'' (1.6 kpc) southwest of the nucleus is associated with highly
blueshifted emission lines seen in ground-based spectra. We interpret the
V-shaped feature as emission from gas compressed by the bow shock driven by the
outwardly moving radio plasmoid.
