The galaxy presents an edge-on disk morphology. A distinct central bulge is visible, appearing smoothly rounded and elongated along the plane of the disk. There is a noticeable color gradient, with the central bulge exhibiting a yellowish-orange hue. The disk appears fainter and bluer compared to the bulge, likely indicating populations of younger, hotter stars. No significant signs of ongoing mergers or major disturbances, such as tidal tails or asymmetrical structures, are apparent. The disk presents a smooth appearance with no visible distinct dust lanes. The lack of star formation regions is indicated by the smoothness of the disk and the lack of hotspots. The galaxy's size appears relatively compact.
