The galaxy presents a somewhat irregular morphology. There is evidence of tidal disturbance and likely interaction. A significant portion of the galaxy displays a smoother component, but distinct features suggesting either a merging event or internal disturbance are apparent. The shape is neither perfectly elliptical nor distinctly disc-like, leaning towards an intermediate classification. The color distribution suggests a mix of stellar populations, with some regions exhibiting bluer tones, potentially indicative of ongoing star formation, and other regions appearing redder, which could suggest older stellar populations or dust obscuration. Overall, the galaxy appears to be dynamically active with a mass of around 10^10 solar masses, and it exhibits a moderate level of star formation.
