  The existence of spiral DRAGNs challenges standard galaxy formation theories.
We present the first observation of 0313$-$192, the archetypal spiral DRAGN, at
VLBI resolutions. Spiral DRAGNs are Double Radio Sources Associated with
Galactic Nuclei (DRAGNs) that are hosted by spiral galaxies. 0313$-$192 is an
edge-on spiral galaxy that appears to host a 360 kpc double-lobed radio source.
The core of this galaxy is clearly detected at L, S, and X-bands using the
VLBA, signifying an ongoing active nucleus in the galaxy. This rules out the
possibility that the spiral DRAGN is merely a chance alignment. The radio core
has L$_{1.4\,GHz} \sim 3.0 \times 10^{23}$W Hz$^{-1}$. Radio components are
detected to the South-West of the core, but there are no detections of a
counterjet. Assuming a symmetric, relativistic jet, we estimate an upper limit
to the inclination angle of $\theta \lesssim 72$ degrees. The VLBI-detected
radio jet components are extremely well-aligned with the larger-scale radio
source suggesting little to no jet disruption or interaction with the ISM of
the host galaxy.
