The galaxy presents a flattened, disk-like morphology. It appears to be an edge-on or highly inclined spiral galaxy, with a bright central bulge. The disk exhibits a slightly clumpy structure, with subtle variations in surface brightness suggesting the presence of spiral arm fragments. The color of the galaxy is predominantly bluish-white, indicative of ongoing star formation, particularly within the disk regions. The bulge is comparatively more yellow, suggesting an older stellar population. There appears to be a hint of dust obscuration along the plane of the disk. Overall, the galaxy does not show strong signs of recent major mergers or strong tidal disturbances, though a small area of increased star formation may be the result of a minor disturbance.
