The galaxy exhibits an asymmetrical morphology with a distorted appearance. The main body of the galaxy displays a diffuse, irregular shape. A notable feature is an apparent tidal tail extending outwards, suggesting gravitational interaction. The color gradient indicates varying stellar populations, with bluer regions potentially indicating recent star formation activity and older, redder regions in other parts of the galaxy. Overall, the observed morphology suggests a galaxy undergoing or having undergone a merger or tidal interaction with another galaxy, or with the intergalactic medium. Further spectroscopic analysis is recommended to better understand the nature of the disturbances. 
