The galaxy presents as a slightly inclined, elongated structure. It displays a prominent disk, observed nearly edge-on. The central bulge appears relatively modest in size and has a rounded shape.  Evidence of some disk structure and dust lanes are visible along the major axis. There do not appear to be any tidal tails or other signs of major interaction with another galaxy. The disk exhibits a relatively smooth texture, indicative of a more ordered, less perturbed system. The overall color gradient suggests some ongoing star formation, potentially more prevalent in the disk than in the bulge.
