This galaxy exhibits an irregular morphology, possibly indicative of an ongoing or recent merger event. The central region displays a concentrated, bright core. A plume of material extends outwards from the main body of the galaxy, suggesting tidal interactions. There is a secondary luminous object offset from the galaxy, which could be a tidal dwarf galaxy or another galaxy interacting with the primary galaxy. The overall color suggests a mix of stellar populations, with some regions appearing bluer, indicating younger stars, and others appearing redder, suggesting older stars. There appears to be star formation occurring, although further spectral analysis would be required to confirm this. The disturbed morphology supports a possible merger scenario, which may be triggering this star formation.
