  Radio-loud sources with blazar-like properties, but having a jet that does
not directly point in the direction of the observer are among the most
interesting classes of gamma-ray emitters. These sources are known as
Misaligned Active Galactic Nuclei (MAGN). Understanding MAGN properties is
useful to improve the knowledge of blazar energetics. We searched for new MAGN
candidates among the remaining blazars of uncertain type detected by the Fermi
Large Area Telescope (LAT) using a methodology based on characterizing their
radio morphology. We identified seven new candidates associated with gamma-ray
sources. Their features are consistent with a source with a misaligned
relativistic jet consistent with the definition of MAGN.
