The galaxy appears to be a late-type spiral system, observed nearly edge-on. The disk component is the dominant feature, exhibiting a pronounced dust lane that bisects the galaxy along its major axis, obscuring the galactic center. The disk itself is relatively thin and elongated. The stellar population in the central region appears older, indicated by the yellower hue. Moving outwards from the center, the disk shows bluer regions possibly indicative of more recent star formation, giving rise to the spiral arm structure. Overall, the galaxy seems well-formed and undisturbed, showing no obvious signs of major recent merger events. The galaxy is of moderate size.
