The galaxy presents as an edge-on spiral, exhibiting a prominent central bulge that gradually fades into a much fainter, elongated disk. The bulge dominates the galaxy's overall luminosity, appearing smooth and relatively featureless in the available imagery. The disk is narrow and appears relatively uniform in color, suggesting a lack of prominent spiral arm structure or active star formation regions in the disk component. The galaxy has a noticeable dust lane that obscures the mid-plane of the disk and further attenuates the light from the galactic bulge. The galaxy exhibits no signs of any major disturbances or ongoing merger activity. The galaxy is well-defined with a regular and symmetrical morphology.
