[1][a] With a diameter of approximately 135 kilometers, Ursula is the second-largest known impact feature on Titania, after Gertrude.

[3] The crater has a flat floor, and Ursula has what appears to be a central pit with diameter of about 20 km.

However, the structure is more likely to be a series of depressions due to multiple tectonic faults breaking up the crater floor.

Though the smooth plains could represent an ejecta blanket, with material blasted out from the impact event that created Ursula obliterating nearby craters, the lack of similar deposits around Titania's other large craters suggest a cryovolcanic origin.

This makes the regions surrounding Ursula one of the only identified candidate cryovolcanic features on Titania, and may be analogous to the smooth plains of Saturn's moons Dione and Tethys.