The galaxy presents as a slightly inclined, disk-like structure. It exhibits a central bulge that appears relatively smooth and concentrated, with a yellowish-orange hue, suggesting an older stellar population. The outer regions of the disk show a bluer color, potentially indicating ongoing star formation within spiral arms. There are some disturbances within the disk, but not extreme. The galaxy's morphology seems to be that of a spiral galaxy, but further investigation would be needed to confirm whether it has a bar, the number of spiral arms, and the degree to which the arms are tightly wound or loosely structured. No obvious signs of a major merger are visible, though minor disturbances may be present within the galactic disk.
