The galaxy presents as a disturbed system, exhibiting significant morphological irregularity. There appears to be ongoing or recent merger activity influencing its structure. A central, brighter region is visible, which likely represents a galactic nucleus or a region of concentrated stellar density. From this central point, a somewhat disrupted arm or tidal tail extends outwards, indicative of gravitational interaction. The light distribution suggests a complex interplay of stellar populations, potentially influenced by the interaction. The overall shape leans towards a disk, although heavily distorted. A slight color gradient may be present, with bluer tones possibly indicating areas of more recent star formation. 
