The galaxy appears to be a spiral galaxy, observed at a near edge-on orientation with respect to our line of sight. A prominent dust lane bisects the galactic disc along the major axis, obscuring a significant portion of the central bulge. The central bulge is subtly visible, exhibiting a smooth and concentrated light profile. Faint spiral arm structures are discernable extending from the central region. The spiral arms do not appear to be tightly wound, and exhibit a degree of patchiness in the star formation regions along the arms. The galaxy displays a bluer color in the outer regions of the disc, indicative of younger stellar populations and active star formation. There is an indication of minor disturbances in the galaxy morphology, however no indication of a recent major merger is present.
