  {\it Hubble Space Telescope} (\hst) Wide Field Planetary Camera 2 ({\it
WFPC2}) images of the Virgo Cluster dwarf elliptical galaxy VCC 128 reveal an
apparently double nucleus. The two components, which are separated by $\sim 32$
pc in projection, have the same magnitude and color. We present a spectrum of
this double nucleus and show that it is inconsistent with one or both
components being emission-line background objects or foreground stars. The most
likely interpretation is that, as suggested by \citet{lauer_etal_96} for the
double nucleus in NGC 4486B, we are seeing a nuclear disk surrounding a
supermassive black hole. This is only the second time an early-type dwarf
(dE/dSph) galaxy has been suggested to host a SMBH.
