A steep-walled, winding channel a few kilometers wide (Anuket Vallis) breaks through the rough terrain surrounding the crater rim.
[5][7] A volcanic origin initially was supported due to non-impact geologic aspects, such as having a low rim, a surrounding plains-forming unit, and a non-concentric nature of its inner basin, as well as its proximity to Maxwell Montes.
[12] Using photogeologic analysis, the floor of the crater has a shallow central depression resulting from subsidence of uplifted mantle material from below due to "viscous relaxation".
[14] This was found in Venusian craters larger than 70 km in diameter by using altimetry data which shows surfaces with different elevations from the Magellan mission.
[6] This results in the melting of the lower levels of the thickened crust and potential magmatic activity, volcanism, and caldera formation at the surface.
[6] The following evidence from Schaber et al.[11] was the leading explanation for a volcanic origin for twelve years until Magellan imagery was returned in the early 1990s.