The galaxy presents a flattened, disk-like structure with a brighter, concentrated central region, suggestive of a bulge or nucleus. The light distribution is not perfectly smooth; some irregularities are observed in the outer regions of the disk. Faint spiral arm-like structures are difficult to resolve from this image alone. The galaxy exhibits an overall blue-green hue. This suggests a population of younger, hotter stars. The observed color gradient indicates a possible radial change in stellar populations or dust content, with potentially redder populations further out. There is a point source that may be a background galaxy or object. The galaxy appears to be relatively undisturbed.
