The galaxy presents a complex morphology, appearing to be undergoing a significant interaction or merger event. There's a central, bright, relatively smooth component with a diffuse, elongated shape. This could be indicative of a spheroidal component, possibly an elliptical galaxy. Adjacent to this is a more disturbed area with hints of disk-like structure, displaying bluer colors and clumpy regions, which may suggest ongoing star formation activity. A faint tidal tail or bridge of material seems to extend from the central, smooth component, connecting to the disturbed region, further supporting the interaction scenario. The overall color indices suggest a mixed stellar population, with some regions exhibiting older, redder stars and others exhibiting younger, bluer stars, typical of a system experiencing recent or ongoing starbursts due to the interaction. The system exhibits significant asymmetry, indicating that the galaxy is likely not in a state of equilibrium. It appears to be a moderate mass system with a moderate rate of star formation.
