  We investigate the predictions of Einsteinian Cubic Gravity (ECG) for the
lensing effects due to supermassive black holes at the center of Milky Way and
other galaxies. Working in the context of spherical symmetry, we obtain the
metric function from a continued fraction method and find that both time delays
and the angular positions of images considerably deviate from general
relativity, as large as milliarcseconds. This suggests that observational tests
of ECG are indeed feasible.
