The galaxy presents a disturbed morphology, possibly indicative of an ongoing or recent interaction. It exhibits an elongated shape with a brighter, more compact central region and a fainter, extended component stretching outwards. The central region appears bluish-white, suggesting the presence of younger, hotter stars. In contrast, the extended structure appears more reddish-orange, indicating older stellar populations or significant dust obscuration. A faint tidal tail is visible on the right side of the galaxy, providing further evidence for gravitational interaction. Overall, the structure of the galaxy suggests a complex evolutionary history, likely involving mergers or tidal interactions with another galaxy. 
