Slicing through the quiet, northern reaches of Canes Venatici, roughly one and a half degrees south-southwest of magnitude-4.3 Beta Canum Venaticorum, NGC 4111 is a brilliant, edge-on lenticular galaxy that stands as a true visual masterpiece for double-star and galaxy enthusiasts alike. Shining around magnitude 10.7, it immediately catches the eye in a 4-inch refractor at low power as a razor-sharp, needle-thin sliver of silver light oriented north-northwest to south-southeast. What elevates the view into an unforgettable star-field portrait is its position embedded within a striking, wide trio of 9th- and 10th-magnitude field stars that frame the galaxy like cosmic bookends.
Pushing the magnification to 120 in a medium-aperture scope reveals the galaxy's dramatic profile in crisp detail. The galaxy’s central core bulges prominently into a bright, compact oval that cuts sharply across the view, while its narrow, whisker-like ray extensions stretch out nearly 4 arcminutes into the ink-black background. Patient observers using gentle averted vision will notice how intensely the central core shines compared to the faint, wispy tips of the spindle, giving NGC 4111 the distinct appearance of a tiny, distant celestial dagger suspended among the stars.
In an 8- or 10-inch reflector at 180x under dark, transparent skies, NGC 4111 reveals its surrounding cosmic neighborhood with stunning clarity. The central hub takes on a brilliant, almost stellar nucleus anchored inside a dense, lens-shaped envelope, while its slender extensions taper gracefully into the void. Larger apertures also unlock a delightful galactic bonus: just 12 arcminutes to the southwest lies the fainter, edge-on spiral neighbor NGC 4117, allowing both galaxies to share a single high-power field of view—a serene, contrasting pair of island universes hovering together in the spring night.