This galaxy exhibits a flattened, disk-like morphology. The primary color is a vibrant blue, with a brighter, almost white, central region, suggesting a concentration of younger, hotter stars in the core. The blue disk fades in intensity moving outward.

There are hints of possible disturbance along the edges of the disk, manifesting as slight irregularities or faint extensions of light beyond the main structure. The overall smooth appearance of the disk suggests a relatively evolved system, although the blue color indicates ongoing star formation. A slight asymmetry in the light distribution is present but not overtly indicative of a major merger event, it may point to a minor interaction or internal dynamical processes.
