The galaxy presents as a highly inclined, disk-shaped structure. A prominent dust lane bisects the galaxy along its major axis, obscuring the central bulge region. The bulge appears small and rather faint. The disk appears elongated, with a bright central region that decreases in luminosity toward the edges. The galaxy exhibits a reddish hue, potentially indicating an older stellar population and moderate levels of recent star formation. There are no indications of a spiral arm structure, with the disk appearing relatively smooth. The overall morphology suggests a late-type spiral or an edge-on lenticular galaxy. No obvious signs of tidal disturbances or interactions are present, though the slight distortions to the disk could be indicative of a minor merger event.
