The galaxy presents a slightly elongated, irregular morphology. The light distribution appears relatively smooth across the main body of the galaxy, yet there is a suggestion of some features or a possible disk-like structure. There appears to be at least two main concentrations of light, possibly indicating a recent or ongoing interaction or merger event. These concentrations are connected by what appears to be tidal features. The galaxy exhibits a blue-ish hue, suggesting a population of younger, hotter stars and possibly recent star formation activity. The galaxy doesn't appear perfectly smooth, but doesn't seem to be a large spiral galaxy. There also seems to be ongoing merging activity between two larger bodies in the system.
