  We observed the quadruple gravitationally lensed image of MGJ0414+0534 on 23
November 1997 with a global VLBI array at 8.4 GHz. We report wide-field imaging
results of its four components at submilliarcsecond resolution, displaying
complex core-like and jet-like extended structures. A simple model combining a
singular isothermal ellipsoid to represent the main lens galaxy, external
shear, and a singular isothermal sphere to represent an additional, nearby
object accounts well for the core positions and flux densities of the VLBI
images. This model predicts delays between the different lensed images of
several weeks.
