  We present 1,201 galaxies at $0.05<z<0.45$ that host tidal features, detected
from the first $\sim\! 200$ deg$^2$ of imaging from the Hyper Suprime-Cam
Subaru Strategic Program (HSC-SSP). All galaxies in the present sample have
spectroscopic observations from the Sloan Digital Sky Survey (SDSS)
spectroscopic campaigns, generating a sample of 21208 galaxies. Of these
galaxies, we identify 214 shell systems and 987 stream systems. For 575 of
these systems, we are additionally able to measure the $(g-i)$ colors of the
tidal features. We find evidence for star formation in a subset of the streams,
with the exception of streams around massive ellipticals, and find that stream
host galaxies span the full range of stellar masses in our sample. Galaxies
which host shells are predominantly red and massive: we find that observable
shells form more frequently around ellipticals than around disc galaxies of the
same stellar mass. Although the majority of the shells in our sample are
consistent with being formed by minor mergers, $15\% \pm 4.4\%$ of shell host
galaxies have $(g-i)$ colors as red as their host galaxy, consistent with being
formed by major mergers. These "red shells" are additionally preferentially
aligned with the major axis of the host galaxy, as previously predicted from
simulations. We suggest that although the bulk of the observable shell
population originates from fairly minor mergers, which preferentially form
shells that are not aligned with the major axis of the galaxy, major mergers
produce a significant number of observable shells.
