This galaxy presents as a flattened, disk-shaped system, observed nearly edge-on from our line of sight. A prominent central bulge is apparent, appearing brighter and more concentrated than the surrounding disk. The bulge exhibits a yellowish hue, suggesting an older stellar population, with minimal dust obscuration. The disk component, while appearing smooth, displays a faint bluish tint. No spiral arm structure is readily discernible, possibly due to the edge-on perspective. There are no signs of major merger activity.
