The galaxy presents as a disk galaxy seen edge-on. A prominent dust lane bisects the galaxy, obscuring the central bulge. The central region appears yellowish, possibly indicative of an older stellar population or dust extinction. Fainter, bluish light is visible in the outer disk, potentially suggesting the presence of younger, hotter stars associated with ongoing star formation. There are no obvious signs of strong tidal disturbances or a major merger event. The galaxy appears relatively smooth and undisturbed in its overall structure.
