Quick Answer: Yes — It's a Pale Blue-Green Disk
Yes, you can see Uranus with a telescope — and it is immediately identifiable even at low magnification by its distinctive pale cyan colour. Unlike the bright white of Venus, the ruddy orange of Mars, or the yellow-white of Jupiter and Saturn, Uranus appears as a small, steady blue-green disk — the result of methane in its atmosphere absorbing red wavelengths and reflecting blue-green light.
Uranus is technically visible to the naked eye under extremely dark skies (magnitude 5.7 in 2026, on the edge of human visibility), but in practice, it is much easier to locate with binoculars or a finder scope. Through any telescope at 60×–100×, Uranus shows a tiny but unmistakable disk — the transition from a point source to a disk is the moment you know you have found it. A 130mm+ telescope under good conditions reveals the planet's subtle atmospheric banding and, on rare occasions at very high magnification (200×+), the faint ring system (discovered only in 1977) as an infinitesimally thin line around the disk.
Uranus reaches opposition in November 2026, when it is closest to Earth (approximately 2.75 billion km) and visible all night. This is the best time to observe it.