The object presents as a late-type galaxy, seen nearly edge-on. A prominent dust lane bisects the galactic disk along its major axis, obscuring the central bulge region. The galaxy exhibits a relatively smooth disk morphology, with some apparent clumping suggestive of star forming regions. The dust lane appears slightly warped. The color profile suggests a higher concentration of older stellar populations towards the galactic bulge, with younger, bluer stars populating the disk, although this is difficult to discern due to the edge-on orientation. There are no obvious signs of a major merger or significant tidal disturbances. Overall the galaxy appears relatively isolated and undisturbed.
