Messier 66 is a intermediate spiral galaxy. It has a weak bar and a loosely wounded spiral structure. The galaxy has striking
dust lanes and bright star clusters along its spiral arms. It also has a well-developed central bulge. The
isophotal axis ratio is 0.32, indicating that it is being viewed at an angle. The galaxy has a high rate of star formation occurring in the spiral arms. Its rate of star formation is about 0.05 solar masses per year. These young stars
ionize their surrounding environment.
Interaction Gravitational interaction from its past encounter with neighboring
NGC 3628 has resulted in an extremely high central mass concentration and a high
molecular to
atomic mass ratio. This also resulted in a resolved non-rotating clump of
H I material apparently removed from one of the
spiral arms. The latter feature shows up visually as an extremely prominent and unusual spiral arm and dust lane structures as originally noted in the
Atlas of Peculiar Galaxies. ==Supernovae==