The galaxy appears to be a spiral galaxy, observed nearly edge-on. There is a clear central bulge, elongated along the major axis of the disk. The bulge exhibits a slight boxy shape, which may be due to bar instabilities or a merger in the past. The disk presents a somewhat smooth texture with some regions of apparent dust absorption visible as darker regions. The overall color gradient suggests a decreasing presence of young, star-forming regions from the center to the outer disk, or higher dust extinction further from the galactic center. There is no obvious presence of any tidal tails or major morphological disturbances, although there may be a minor disturbance present in the disk.
