The galaxy presents an irregular morphology, suggestive of an ongoing or recent interaction. Two distinct luminosity peaks are observed. One is a brighter, yellowish core, and the other is a bluer, slightly less luminous region, offset from the core. The overall light distribution indicates an extended halo or envelope. Wispy structures are evident emanating from the central regions, hinting at tidal features or disrupted spiral arms. A slight asymmetry is observed in the outer regions, further supporting the disturbed nature of this system. Overall, the appearance suggests a merger or interaction between two galaxies of unequal mass. The absence of well-defined spiral arms and the presence of the aforementioned features imply an advanced stage of merging.
