The galaxy exhibits an overall elliptical morphology, although there is a clear indication of tidal disturbance or a possible ongoing merger event. The core of the galaxy appears smooth and concentrated. There are two distinct luminous regions visible, suggesting the presence of two galactic nuclei or centers of mass. These regions display a yellowish-orange color, potentially indicating an older stellar population or significant dust obscuration. Diffuse light extends outwards from these central regions, creating a faint halo. The galaxy exhibits an irregular shape overall, and the light distribution is not uniform, with some areas appearing brighter and more concentrated than others. There is a visible bridge of light and matter connecting the two central luminous regions. It is possible that the object may also be a single disk galaxy that is seen almost perfectly edge-on. This would explain the apparent double nuclei structure as the light from each edge of the galactic disk is concentrated as we see it. 
