Galaxy Digital (GLXY) Technical Analysis
As of 2026-10-26, GLXY last traded at 15.68 USD (+6.81% on the day) and is in a range on the daily timeframe — insufficient history for 200-DMA. Nearest levels: no clear near support below, 22.65 USD resistance above. 14-day RSI is 23.1 (oversold).
Last updated 2026-10-26 · Source: end-of-day prices (adjusted); indicators computed by SniperIQ
Is GLXY in an uptrend or downtrend?
Galaxy Digital is in a range — insufficient history for 200-DMA.
| Last close | 15.68 USD (+6.81%) |
|---|---|
| 20-day average | 19.224 USD |
| 50-day average | 21.856 USD |
| 200-day average | n/a |
Key support and resistance levels for GLXY
Derived from swing pivots over the last 69 sessions:
| Level | Type | Strength | Touches |
|---|---|---|---|
| 22.65 USD | Resistance | Minor | 1 |
| 24.55 USD | Resistance | Minor | 1 |
| 26.05 USD | Resistance | Minor | 1 |
No clearly-defined swing levels in the current range.
GLXY 52-week range, momentum and volatility
| 52-week high | 36.1 USD (56.6% below) |
|---|---|
| 52-week low | 14.19 USD (10.5% above) |
| 14-day RSI | 23.1 (Oversold) |
| 14-day ATR | 1.5 USD (9.57% of price, High volatility) |
Related research pages
More on GLXY
Frequently asked questions
Is Galaxy Digital (GLXY) in an uptrend or downtrend?
As of 2026-10-26, GLXY is in a range on the daily timeframe — insufficient history for 200-DMA. Last close 15.68 USD vs 50-day average 21.856 USD and 200-day average n/a.
What are the key support and resistance levels for GLXY?
No clear support below price in range. Nearest resistance is around 22.65 USD (minor). Levels are derived from swing pivots over the last ~200 sessions.
What is GLXY's 52-week high and low?
Over the last 52 weeks, GLXY traded between 14.19 USD and 36.1 USD. It is currently 56.6% below its 52-week high.
Is GLXY overbought or oversold?
The 14-day RSI is 23.1 — in oversold territory (<30). Momentum reads as oversold.
How volatile is GLXY?
Its 14-day Average True Range is 1.5 (9.57% of price) — high volatility relative to price.