The galaxy appears to be undergoing a significant interaction, possibly a merger. There are at least three distinct luminous components visible, with the largest suggesting a relatively smooth, round morphology. However, the overall structure of the galaxy is irregular and disturbed. There is evidence of tidal features, but it is difficult to clearly distinguish them from the general background noise. The light emitted from the galaxy is primarily concentrated in a few bright areas, with some indication of fainter, diffuse emission extending beyond these cores. The relative brightness of the components suggests that they are at different distances, or may be experiencing localized star formation. The colors suggest that the galaxy contains a population of young, hot stars and the absence of any redder light hints that the galaxy is not particularly dusty, and old stars are not very common.
