The galaxy presents a complex morphology, suggestive of an ongoing or recent interaction or merger event. The primary structure appears to be a relatively smooth, centrally concentrated body. There is a distinct, secondary concentration of light that may represent a separate galactic nucleus or a region of enhanced star formation triggered by the interaction. 

The color gradient within the galaxy ranges from bluer hues in the less concentrated, outer regions to redder tones toward the apparent center. The overall shape is generally rounded. There are some faint signs of disturbances in the overall structure, which could be tidal tails or bridges indicative of gravitational interaction. Overall, the morphology suggests a significant disturbance to its overall form.
