Several features can be seen in this Mars image. Particularly striking is Solis Lacus surrounded by the prominent Thaumasia to the South. Also striking is Tithnius Lacus and its subtle albedo extension of Noctis Lacus.
Juventae Fons is quite prominent. What is interesting is the prominent albedo (arrowed) seen extending from Niliacus Lacus (NL) towards Sinus Meridiani (SM). This extension is normally not captured as extending from NL but instead from SM. Could this be some artifact or due to some more transparent conditions over that part of the planet?
There are no other diminished albedo features that suggest the occurrence of any dust storms.