The galaxy presents as a disk-shaped structure, viewed nearly edge-on from our perspective. The primary component is a bright, elongated central bulge with a yellowish-white hue, suggesting a population of older stars. A faint, flattened disk extends outwards from the bulge. The galaxy's disk exhibits a subtle dust lane along the plane of symmetry, hinting at the presence of interstellar material. The overall color gradient suggests a transition from a bluer disk to a redder, more evolved bulge. There may be some minor disturbances within the galaxy, or it is fairly relaxed in its structure.
