The galaxy appears to be undergoing a significant merger or interaction, displaying a complex and disturbed morphology. There are two distinct regions of concentrated light, suggesting either two interacting galaxies or the remnant nucleus and a tidal dwarf galaxy. A faint, diffuse stream of stellar material is evident, extending outwards from the main body of the galaxy, indicative of tidal forces at play during a merging event. The color distribution is relatively heterogeneous, with bluer regions possibly indicating active star formation areas, and redder regions likely older stellar populations. Overall, the galaxy is likely in a late stage of interaction, where components are highly disrupted, and tidal features are becoming prominent.
