The observed galaxy presents a clear spiral morphology. Two prominent spiral arms emanate from a bright, moderately sized central bulge. The spiral arms exhibit a relatively loose winding pattern. The galaxy's disk appears to be oriented close to face-on, as indicated by its near-circular projected shape. The arms are somewhat flocculent. There is no obvious bar structure visible within the central region. No signs of a major ongoing merger or strong tidal disturbance are apparent.
