The galaxy exhibits a disturbed morphology. It is elongated in shape, appearing cigar-like. A bright central bulge is observed, exhibiting a yellow-orange hue, potentially indicating an older stellar population. Extending away from the bulge is a region of bluer light, possibly suggesting ongoing star formation within a disrupted or tidal feature. The overall structure suggests a possible interaction or merger event, with apparent tidal tails or other disturbances extending from the main body of the galaxy. The presence of a merging signature cannot be ruled out. 
