This galaxy appears to be an edge-on spiral galaxy, presenting a flattened, elongated morphology. It exhibits a prominent central bulge that appears relatively smooth and rounded, displaying a yellowish color, suggesting an older stellar population. The disk component, viewed edge-on, shows a more diffuse, bluish-white hue, indicative of ongoing star formation. There is some indication of dust lanes along the galactic plane, but they are not sharply defined. Overall, the galaxy seems well-ordered, lacking any obvious signs of major disturbances or ongoing merging activity. The color gradient suggests the presence of a stellar population gradient within the galaxy.
