The galaxy exhibits a disturbed morphology, suggesting ongoing or recent interaction or merger activity. The overall structure appears elongated with a bright central region. There is a noticeable color gradient across the galaxy, with a yellow to orange hue concentrated in the central region, possibly indicative of an older stellar population or significant dust obscuration. The outer regions display a bluer color, which could indicate the presence of younger, hotter stars and ongoing star formation. There appear to be tidal features, possibly faint streams or tails extending from the main body of the galaxy, further supporting the interaction/merger hypothesis. These features are less defined but suggest gravitational disruption. Overall, the galaxy shows signs of significant recent dynamical activity and a diverse stellar population.
