This galaxy presents a flattened, somewhat amorphous morphology, suggesting it may be an irregular or a late-type spiral galaxy seen at an oblique angle. The central region exhibits a brighter, more concentrated luminosity, possibly indicating a bulge or a central concentration of stars. The overall color of the galaxy appears bluish, indicating the presence of younger, hotter stars. The structure of the galaxy seems disturbed. This could be due to tidal interactions or past mergers. There appears to be some ongoing star formation within the galaxy, as evidenced by the blue coloration, but this activity seems relatively subdued. There are hints of a disk structure, but the light distribution is not uniform, displaying some clumpy regions that could be stellar associations or HII regions.
