The galaxy presents with an apparently disturbed morphology. It shows evidence of a tidal interaction or possible ongoing merger event. The main galactic body appears elongated with a bright, centrally located core region that shifts to a yellowish color, which could possibly indicate a greater concentration of older stars or dust obscuration. Extending from this core are diffuse arms, exhibiting a fainter bluish component, which might suggest areas of recent star formation activity. One arm appears more prominent, extending further and displaying a mottled texture. Overall, the galaxy does not present a smooth, elliptical profile, but rather a more complex structure indicative of dynamical processes influencing its morphology. There is possibly another object interacting with the main galaxy. 
