The galaxy presents a morphology indicative of a system undergoing a significant interaction or merger. The light distribution appears relatively smooth in some areas, with evidence of disturbances throughout.

The primary body of the galaxy shows an irregular shape. There are two distinct bright components, each appearing as a prominent concentration of light. These bright regions may be the nuclei of the merging galaxies.

Color gradients are visible within the galaxy. The central regions and components exhibit a more reddish hue, potentially indicating an older stellar population and/or significant dust obscuration. The outer regions appear somewhat bluer, suggesting the presence of younger stars and ongoing star formation. However, the overall color is generally red, suggesting an elliptical classification.

There is a low signal-to-noise ratio in the image, resulting in a blurry morphology.
