The galaxy presents as a disk galaxy, though its features are significantly disturbed. A central bulge is visible, exhibiting a yellowish-orange hue, potentially indicating an older stellar population. The surrounding disk appears clumpy and irregular, with hints of spiral structure disrupted by what appears to be a major merger event. The overall color suggests active star formation, mixed with regions of older, redder stars. There is morphological evidence of a significant interaction or recent merger impacting the galaxy's structure, including a tidal tail or plume extending away from the main galactic body. The galaxy has a flattened shape, and the overall morphology is indicative of a system undergoing significant gravitational disturbance.