The galaxy presents as an edge-on spiral, exhibiting a prominent disk structure. A central bulge appears present. Evidence of dust lanes is strongly suggested by the dark band bisecting the galactic plane. The outer disk appears somewhat disrupted or irregular, implying potential gravitational interactions. The galaxy displays a color gradient, transitioning from bluer hues in the outer disk to redder tones in the central bulge, indicative of differing stellar populations. The overall morphology hints at a high probability that the galaxy is an undisturbed, although possibly actively star-forming, system.
