The galaxy presents as a spiral disk, observed nearly edge-on. A dust lane bisects the galaxy, obscuring a significant portion of the galactic plane. The stellar population appears relatively old, emitting light at a redshift of approximately 0.295. The overall color indices suggest a moderate amount of star formation, although current activity is low and the galaxy is not considered to be rapidly forming new stars. No prominent signs of interaction with other galaxies are evident, the galaxy appears isolated and undisturbed. There is no significant galactic bulge. Overall, the morphological classification favors an edge-on spiral galaxy of considerable mass.
