This 70 km-wide crater shows interesting internal features, including a smaller crater (foreground), exposed light-toned deposits (foreground/centre), and chaotic terrain (background), as well as slumped crater walls.
The oblique perspective view was generated using data from the Mars Express high-resolution stereo camera stereo channels. This scene is part of the region imaged on 13 March 2007 and 22 February 2017 during orbits 4090 and 16648. The image mosaic is centred on 346°E/23°S, with a ground resolution of 15–17 m/pixel.