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This paper presents a morphology classification catalog of spiral and ringfeatures of 59,854 magnitude-limited galaxies ($r<17.8$ mag, and additional628,005 subsamples down to $r=20$ mag) at $z=0.01-0.3$ based on the ThirdPublic Data Release of the Hyper Suprime-Cam Subaru Strategic Program. Weemploy two deep learning classifiers to determine the spiral and ringstructures separately based on GALAXY CRUISE Data Release 1, which is dedicatedto Hyper Suprime-Cam data. The number of spiral and ring galaxies contain31,864 and 8,808 sources, respectively, which constitute 53\% and 15\% of thesample. A notable result of this study is the construction of a large sample ofring galaxies utilizing high-quality imaging data delivered by the Subaru HyperSuprime-Cam. However, the accurate identification of ring galaxies remainsdifficult at a limited seeing resolution. Additionally, we confirm that mostspiral galaxies are located on the star-forming main sequence, whereas ringgalaxies preferentially reside in the green valley at stellar mass of$10^{10.5}-10^{11}$ solar mass. Furthermore, decreasing fractions of spiral andring galaxies are observed toward the centers of the galaxy clusters. Theobtained morphology catalog is publicly available on the GALAXY CRUISE website.

GALAXY CRUISE: Spiral and ring classifications for bright galaxies at z=0.01-0.3