This looks like water erosion to my IANAG¹ eyes. Some papers have suggested the existence of thermal springs in the aftermath of the Jezero meteor impact.

Over-processed, leveled, cropped MCZ_RIGHT, FL: 110mm
looking ESE (107°) from RMC 82.2866
Sol 1706, LMST: 13:38:46
Original: https://mars.nasa.gov/mars2020-raw-images/pub/ods/surface/sol/01706/ids/edr/browse/zcam/ZR0_1706_0818393954_428EBY_N0822866ZCAM04289_1100LMJ01.png

Credit: #NASA/JPL-Caltech/ASU/65dBnoise

¹ IANAG = I Am Not A Geologist

#Perseverance #Mars2020 #Solarocks #Space

@65dBnoise Note that fluvial features needn't be those of water, anything naturally transitioning into a liquid phase or undergoing periodic, e.g. diurnal phase transitions will do. In case of Mars, with its extremely low surface temperatures and a very tenuous atmosphere, that could also be carbon dioxide undergoing regular deposition into dry ice, sliding down steeper slopes in its solid state and then sublimating back into its gaseous phase, one such cycle between the other sides of cabon dioxide's triple point every Sol. I'm not saying that's the case here, just that it's a possibility (that glacial features can look very similar to fluvial ones) that would need to be considered before drawing conclusions.

@tildalwave
Thanks for the comment. Indeed that seems to have been the case with a number of similar features elsewhere on Mars. The reason I mention water and thermal springs though is because it's mentioned frequently in papers as having played a role in shaping rocks and terrain inside and around Jezero Crater.

@sharponlooker's curated hashtag #JezeroRimScience has been very helpful in collecting papers about the subject and is worth having a look.