This galaxy presents as a flattened, disk-like structure, viewed edge-on or at a highly inclined angle. The central region appears brighter and more concentrated, suggesting a bulge, potentially harboring an older stellar population. The overall color of the galaxy is slightly blue-ish near the edges and more yellowish-white towards the center. This could indicate ongoing star formation in the outer regions, possibly tracing spiral arms that are difficult to discern due to the edge-on view. Faint dust lanes or obscuring material might be present within the disk, causing subtle variations in the light distribution. No obvious signs of major mergers or strong tidal disturbances are visible. It appears to be a relatively undisturbed and isolated system.
