The galaxy presents a generally smooth morphology, though a slight asymmetry is observed. It exhibits a predominantly round shape, deviating minimally from circularity. The color distribution indicates a central concentration of bluer light, possibly indicative of younger stellar populations or active star formation within the core. The outer regions appear relatively diffuse, exhibiting a gradual decrease in intensity with radial distance. There is a hint of minor disturbance in the form of a faint, extended feature on one side of the galaxy, this could be a faint tidal tail, suggesting a possible past interaction with another galaxy. No clear spiral arms or bar structures are discernible in the available image.