  The discovery of SN 2002ic and subsequent spectroscopic studies have led to
the surprising finding that SN 2002ic is a Type Ia supernova with strong
ejecta-circumstellar interaction. Here we show that nearly 1 year after the
explosion the supernova has become fainter overall, but the H$\alpha$ emission
has brightened and broadened dramatically compared to earlier observations. We
have obtained spectropolarimetry data which show that the hydrogen-rich matter
is highly aspherically distributed. These observations suggest that the
supernova exploded inside a dense, clumpy, disk-like circumstellar environment.
