Lower parts of the surface are shown in blues and purples, while higher-altitude regions show up in whites, browns, and reds, as indicated on the scale to the top right. The crater’s thick deposit of ice can be seen at the centre of the frame.

This view is based on a digital terrain model of the region, from which the topography of the landscape can be derived. It comprises data obtained by the High Resolution Stereo Camera on Mars Express over orbits 18042 (captured on 4 April 2018), 5726, 5692, 5654, and 1412.It covers a region centred at 165° E, 73° N, and has a resolution of approximately 21 metres per pixel.