The galaxy presents as an edge-on spiral. There is a prominent central bulge, which appears smooth and relatively bright, suggesting a concentration of older stars. The disk is visible as a flattened structure extending outwards from the bulge. The disk is relatively smooth with hints of darker dust lanes, giving a non-uniform appearance. The overall color of the galaxy is yellowish-white, which could indicate a population of stars with intermediate ages. There are no strong indications of active star formation regions from the available image, and no signs of any tidal tails or significant disturbances suggesting any recent major merger event. The smooth appearance indicates that the galaxy is relatively evolved, with possible recent minor disturbance.
