The galaxy appears to be in a late stage merger. Two distinct nuclei are observed within a common, disturbed halo. One nucleus shows bluer color, suggesting ongoing or recent star formation activity. The other nucleus is redder in color, suggesting an older stellar population and less active star formation. A tidal bridge is visible, connecting the two merging galaxies and indicating gravitational interaction. The overall morphology is highly irregular and complex, typical of merging systems. There are hints of tidal tails extending outwards, indicative of significant gravitational disruption. Given the redshift of 0.080019, the galaxy is relatively nearby.
