The observed galaxy presents a morphology suggesting an ongoing or recent merger event. The primary galactic body exhibits a relatively smooth and round structure, with a concentrated central bulge. A secondary, smaller structure is observed in close proximity, potentially representing a satellite galaxy in the process of tidal disruption. There is evidence of tidal tails or bridges extending between the two structures. The overall color of the galaxy leans toward the redder end of the spectrum, indicative of an older stellar population and potentially lower rates of star formation. The galaxy displays a moderate level of asymmetry, potentially caused by the gravitational interactions of the ongoing merger.
