  We report photometric and spectroscopic observations of the 2014 eclipse of
EE Cep. This proved to be one of the shallower eclipses on record rather than
one of the deepest as predicted. The general shape of the eclipse light curve
was similar to that of the 2003 eclipse. The spectral type before and after
eclipse was consistent with B5III and became slightly later at mid-eclipse.
Total flux in the H{\alpha} emission line remained relatively constant through
the eclipse.
