An interaction of dust particles with R = 0.168 μm, ϱ = 1 g cm^-3 and ejected from parent bodies in the debris ring around HD 61005 located between 55 and 65 AU and the interstellar wind with number densities n_H = 80 cm^-3, n_He = 6 cm^-3, and n_p = 12.8 cm^-3 moving perpendicularly to the debris ring with relative velocity 30 km s^-1 with respect to the star. Color-scale is linear with observed intensity of light with wavelength λ = 580 nm scattered on the dust particles according to Mie scattering theory. The ring mid-plane is located in the xy-plane. The bottom-left plot is created by a rotation of a viewpoint in the top-left plot by the angle 45° counterclockwise around x-axis in yz-plane. The bottom-right plot is created by the rotation of a viewpoint in the top-left plot by the angle 95.7° counterclockwise around the x-axis in yz-plane in order to show the shape morphology observed from the Earth.