This galaxy appears to be in the process of a significant interaction, possibly a merger. The overall morphology is irregular, lacking a distinct spiral arm structure or elliptical profile. There appear to be multiple luminous cores or concentrations of light, suggesting the presence of multiple galactic nuclei, or regions of intense star formation triggered by gravitational interactions. A tidal tail or bridge appears to be either non-existent or faint and obscured. Color gradients are subtle, but it appears to be dominated by redder colors overall. The isophotes are likely not smooth and continuous, indicating asymmetries and possibly tidal features associated with the interaction. A smooth central component is less apparent in comparison to distinct individual luminous components. The observed structure is consistent with a system undergoing a major or ongoing merger, although further spectroscopic or high resolution data would be necessary to confirm this assessment.
