The galaxy exhibits an irregular morphology, indicative of an ongoing or recent merger event. The primary structure appears relatively smooth, but displays noticeable disturbances and tidal features. A prominent feature is the presence of two distinct nuclei, with the western nucleus exhibiting a yellow-orange hue and the eastern nucleus appearing bluer, possibly due to higher star formation. There is evidence of tidal tails and disrupted structures emanating from the central regions, suggesting gravitational interaction. The overall color is a mix of yellow and blue, suggesting a combination of older stellar populations and regions of active star formation. The light distribution is not perfectly symmetric. The overall shape does not appear perfectly round, but rather somewhat elongated. There is a significant disturbance in the general structure of the galaxy.
