The galaxy presents as a merging system or a galaxy exhibiting significant tidal disturbances. It appears to comprise at least two distinct luminous cores, suggesting ongoing or recent merger activity. The overall morphology deviates significantly from a regular elliptical or spiral structure, showing an irregular shape with no clear disk-like structure.

The light profile appears smooth, with one core slightly brighter than the other. The color is a broad yellow-white indicative of an intermediate age stellar population, and potentially suppressed star formation. The outer regions of the galaxy display a more diffuse structure, extending beyond the central concentration of light, implying the presence of a stellar halo or tidal debris resulting from gravitational interactions. The colors shift slightly towards red in the halo, suggesting the possibility of an older, redder stellar population in that region.
