This galaxy appears to be a spiral galaxy viewed at a high inclination angle, nearing edge-on. A prominent central bulge, exhibiting a yellow-orange hue, dominates the galaxy's core region. The disk is visible, displaying a bluer color extending away from the central bulge, suggesting the presence of younger, hotter stars and ongoing star formation within the galactic arms. The galaxy does not appear to show signs of a recent major merger, although there is evidence of some distortions within the disk, potentially indicative of minor gravitational interactions or internal dynamic processes. Patches of dust are seen primarily in the lower regions of the galaxy. The overall structure suggests a fairly evolved spiral system.