The galaxy presents a morphology indicative of a system undergoing, or having recently undergone, a significant interaction or merger. The primary structure shows a somewhat amorphous, centrally concentrated bulge, exhibiting a yellowish-white color, suggesting an older stellar population. Emanating from this central region are faint tidal features, potentially indicating streams or disrupted arms. There is an elongated, less luminous extension which might be a tidal tail. Overall, the galaxy's structure deviates significantly from a standard elliptical or spiral morphology. It appears disturbed with possible recent star formation regions near the core.
