  We measure the starspot radii and latitude distribution on the K4 dwarf
HAT-P-11 from Kepler short-cadence photometry. We take advantage of starspot
occultations by its highly-misaligned planet to compare the spot size and
latitude distributions to those of sunspots. We find that the spots of HAT-P-11
are distributed in latitude much like sunspots near solar activity maximum,
with mean spot latitude of $16 \pm 1$ degrees. The majority of starspots of
HAT-P-11 have physical sizes that closely resemble the sizes of sunspots at
solar maximum. We estimate the mean spotted area coverage on HAT-P-11 is
$3^{+6}_{-1}\%$, roughly two orders of magnitude greater than the typical solar
spotted area.
