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We present the light curve of HS 0229+8016 between 2006 and 2019, which shows that the star varies between magnitudes 13.4 and 15.1. There were episodes lasting up to hundreds of days during which distinctive 0.6mag cyclic variations were apparent, each lasting ~9.5 days. Observationally, these were very similar to the ‘stunted’ outbursts seen from time to time in several nova-like cataclysmic variables, such as UU Aqr. There were two intervals of up to 166 days when these stunted outbursts appeared to reduce or even stop. These coincided with the system being up to ~0.7mag fainter than usual. Previous workers have suggested that HS 0229+8016 might be a member of the Z Cam family of dwarf novae, but we can find no evidence of the characteristic dwarf nova outbursts and standstills at an intermediate brightness. Surveillance of HS 0229+8016 should be continued to understand more about the long-term behaviour of this system.