The galaxy presents as a flattened, elongated structure indicative of an edge-on or highly inclined spiral or lenticular galaxy. A central bulge is evident, exhibiting a yellowish-white hue, suggesting an older stellar population. The disk component shows a gradient from bluer colors toward the outer regions to a more yellow hue as you move closer to the bulge, possibly indicating ongoing, albeit limited, star formation in the spiral arms and disk. The dust lanes are faint, but visible, and cause some slight patchiness throughout the galactic disk. The overall morphology appears relatively undisturbed, lacking significant signs of major mergers or tidal interactions.
