HD 131835 observed in scattered light, using the VLT/SPHERE instrument. The white star at the centre denotes the position of the star. The white bar at the bottom right corner represents a distance of 0.5^′′, with the corresponding value in au. In addition to the scattered light image, the contours of the corresponding ALMA dust continuum observations (thermal emission of bigger dust grains) are plotted. There are three contour levels, corresponding to [3, 5, 7] sigma. The white ellipse at the bottom left represents the beam size for the ALMA observation, using a robust value of 0.3. North is up and east is left.