The galaxy presents as an edge-on spiral, with a prominent disk exhibiting a noticeable dust lane along its mid-plane. This obscuration indicates the presence of significant interstellar material within the disk. The central bulge appears distinct and elongated, possibly containing an old stellar population, evidenced by its yellowish color. The absence of clear spiral arm structure suggests that the galaxy is either a lenticular or a tightly wound spiral galaxy.

Evidence suggests a recent interaction or merger event with a smaller galaxy is present, with possible tidal disturbances. The blue color of the possible secondary galaxy or disturbed area suggests active star formation.
