The galaxy presents as an edge-on spiral, exhibiting a flattened disk morphology. A prominent central bulge is observed, with a smooth, rounded appearance, indicative of a relatively evolved stellar population. The disk displays subtle variations in color, hinting at potential areas of on-going star formation, particularly in the bluer hues located on the galaxy's edges. Dust lanes are suspected, though not clearly resolved, obscuring some of the light from the bulge and inner disk. Overall, the galaxy appears relatively undisturbed, showing no strong evidence of recent major mergers, although a minor interaction cannot be ruled out.
