The galaxy presents as an irregular object with a notable blue hue, suggestive of ongoing star formation. The light distribution is somewhat amorphous, lacking a well-defined central bulge or spiral arm structure. There appear to be two or three distinct regions of higher luminosity within the galaxy's body, potentially indicating concentrations of young, hot stars or active galactic nuclei. A faint, extended halo is visible, though its boundaries are not clearly demarcated. There appears to be a major disturbance occurring within the galaxy. The overall morphology is indicative of a galaxy undergoing a merging event.
