The galaxy presents a clear edge-on disk morphology. A prominent dust lane bisects the galaxy along its major axis, indicative of significant interstellar medium obscuration. The central bulge appears relatively small and concentrated, with a smooth, yellowish hue, suggesting a population of older stars. The disk component exhibits a bluer coloration toward the outer regions, likely due to ongoing star formation. Overall the galaxy appears relatively faint. The galaxy appears to be relatively undisturbed, showing no signs of recent major mergers.
