The galaxy presents as a moderately bright, slightly elongated object. Its overall color appears to be on the bluer end of the spectrum, potentially indicative of a younger stellar population or active star formation. The light profile seems relatively smooth, with a centrally concentrated morphology and a gradual decrease in luminosity moving outward from the core. There is a hint of asymmetry, with a slight tapering on one end, though it is difficult to ascertain a clear disk structure or spiral arm features. The galaxy exhibits a subtle ellipticity. There is no clear evidence of a strong tidal disturbance or an ongoing major merger event in this image.
