  We report the radio continuum structure of the barred galaxy NGC 3367 with an
angular resolution of 4''.5. The radio structure indicates emission from the
disk and from a triple source consisting of the nucleus straddled by extended
sources (the lobes). The triple source shows an excess of radio continuum
emission compared to the emission expected from the total radio - Halpha
correlation, suggesting a non-thermal origin probably related to AGN activity
and no to star formation processes. The triple source is about 12 kpc in
diameter at a P.A. 40, close (but not aligned) to that of the stellar bar P.A.
65. Only the southwest lobe is polarized. The polarizatrion asymmetry between
the two lobes suggests that the triple source axis is slightly out of the
plane.
