The galaxy appears to be a flattened, disk-shaped object, observed edge-on. It exhibits a relatively smooth, centralized concentration of light, likely representing a bulge or core component. This central region displays a yellowish hue, potentially indicative of an older stellar population. A distinct, extended, and relatively thin band of blue light is visible, likely a well-defined galactic disk. The disk color suggests the presence of younger, hotter stars and ongoing star formation.

The overall structure indicates a mature galaxy, not exhibiting obvious signs of a major ongoing merger, though subtle irregularities could point to minor gravitational interactions. The rounded appearance of the central bulge suggests it is relatively undisturbed. There is the possibility of an artifact being mistaken for a morphological feature, as well as a small possibility of a more disturbed morphology.