  In the classic Hubble spiral sequence, arm windiness correlates with bulge
size; Sa type spiral galaxies with larger bulges also have the most tightly
wound spirals. Exceptions to this have long been known, and in recent work
using Galaxy Zoo morphologies no strong correlation was seen in a volume
limited sample. In this Research Note, we explore the impact of galaxy mass and
integrated color upon this correlation in the Galaxy Zoo sample, finding that
bluer and lower mass spirals show the ``expected" correlation; however, it
becomes slightly negative for redder and/or more massive spiral galaxies.
