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We present recent Very Long Baseline Array (VLBA) 5 GHz radio observations ofthe nearby, luminous Seyfert 2 galaxy NGC 1068 for comparison to similar VLBAobservations made on 1997 April 26. By cross-correlating the positions ofemitting regions across both epochs, we find that spatially-resolvedextra-nuclear radio knots in this system have sub-relativistic transversespeeds (v < 0.1c). We discuss sources of the observed knots and how the radioemission relates to additional phases of gas in the central ~150 pcs of thissystem. We suggest that the most likely explanation for the observed emissionis synchrotron radiation formed by shocked host media via interactions betweenAGN winds and the host environment.

No Small Scale Radio Jets Here: Multi-Epoch Observations of Radio Continuum Structures in NGC 1068 with the VLBA