The object appears to be a disk galaxy, observed nearly edge-on. There's a prominent central bulge, elongated along the major axis of the disk, that appears round and not boxy. The disk shows a slight indication of dust lanes or obscured regions, particularly along the central plane. The galaxy appears relatively smooth with no obvious signs of spiral arms or significant star-forming regions. The disk's morphology suggests that this is a mature galaxy, with a relatively low star formation rate. There are no clear signs of ongoing mergers or major disturbances in its structure; only slight indications of possible minor disturbances nearby. The color profile seems to indicate a mixture of older stellar populations.
