The galaxy appears to be a merging system, composed of two distinct galactic nuclei. These nuclei exhibit intense luminosity, with each being surrounded by a diffuse halo of lower surface brightness. There is evidence of a possible tidal bridge or stream connecting the two nuclei, suggesting ongoing gravitational interaction. Both galactic components appear to be exhibiting disturbed morphology, deviating significantly from typical elliptical or spiral structures. There might be a presence of minor disturbances in the outer regions of the galaxy. The overall color profile of the galaxy indicates a mixed stellar population, with both older, redder stars, and younger, bluer stars present.
