Context :

Aims : In 2015 , we initiated a survey of Scorpius-Centaurus A-F stars that are predicted to host warm-inner and cold-outer belts of debris similar to the case of the system HR 8799 .
The survey aims to resolve the disks and detect planets responsible for the disk morphology .
In this paper , we study the F-type star HIP 67497 and present a first-order modelisation of the disk in order to derive its main properties .

Methods : We used the near-infrared integral field spectrograph ( IFS ) and dual-band imager IRDIS of VLT/SPHERE to obtain angular-differential imaging observations of the circumstellar environnement of HIP 67497 .
We removed the stellar halo with PCA and TLOCI algorithms .
We modeled the disk emission with the GRaTeR code .

Results : We resolve a ring-like structure that extends up to \sim 450 mas ( \sim 50 au ) from the star in the IRDIS and IFS data .
It is best reproduced by models of a non-eccentric ring with an inclination of 80 \pm 1 ^ { \circ } , a position angle of -93 \pm 1 ^ { \circ } , and a semi-major axis of 59 \pm 3 au .
We also detect an additional , but fainter , arc-like structure with a larger extension ( 0.65 arcsec ) South of the ring that we model as a second belt of debris at \sim 130 au .
We detect 10 candidate companions at separations \geq 1 ” .
We estimate the mass of putative perturbers responsible for the disk morphology and compare it to our detection limits .
Additional data are needed to find those perturbers , and to relate our images to large-scale structures seen with HST/STIS .

Conclusions :