The galaxy presents a disk-like morphology, viewed at a moderate inclination. A central bulge is visible, exhibiting a smooth, concentrated luminosity profile. The disk component displays a mottled texture, suggestive of spiral arm structures, although these are not sharply defined. Blue hues are apparent along the outer regions of the disk, possibly indicating regions of active star formation. Dust lanes are subtly visible, particularly on the side of the galaxy that appears further away, obscuring some of the light from behind it. The overall color gradient transitions from a more yellowish central bulge to bluer outer regions, indicative of differing stellar populations. The galaxy does not show strong signs of a major ongoing merger, but there may be minor disturbances or interactions influencing its structure.
