The galaxy presents a complex morphology with evidence of significant disturbance, potentially indicative of an ongoing or recent merger event. The central region displays a somewhat amorphous structure, lacking a clearly defined bulge. Diffuse, irregular arm-like features extend outward, exhibiting a clumpy appearance. The presence of these features suggests active star formation. There is a hint of tidal debris or disrupted structures. The overall color profile seems to be on the bluer end of the spectrum, consistent with a population of younger, hotter stars. A weak bar structure appears to be present.
