The galaxy appears as a slightly elongated, disk-shaped structure. It exhibits a smooth, concentrated central bulge, which appears yellow/white, suggesting an older stellar population. Extending outward from the bulge is a fainter, more diffuse disk, appearing greenish-yellow. This suggests some ongoing, though perhaps modest, star formation in the disk. The galaxy does not show any obvious signs of major disturbances or interactions with other galaxies, maintaining a relatively undisturbed morphology. There is a subtle asymmetry with the disk, as it has brighter regions on one side, which may be associated with spiral arm structures. The overall color suggests an intermediate age galaxy that is slowly forming new stars.
