The observed galaxy exhibits morphological characteristics consistent with an ongoing or recent merger event. The primary structure is diffuse, displaying a complex, irregular shape with no readily discernible spiral arms or central bulge. Two distinct, bright, and somewhat rounded central concentrations of light are visible, possibly representing the cores of the merging galaxies. The overall color profile is complex. The central concentrations are yellow-white, indicative of older stellar populations, while peripheral regions appear somewhat bluer, hinting at regions of more recent star formation. There's also evidence of a distinct redder area, which may indicate a heavily dust-obscured region or a population of older, redder stars. The spatial extent of the object appears relatively small. Faint tidal features or extended stellar streams are either absent or obscured in this observation.
