The observed galaxy appears to be undergoing a merger. Two distinct nuclei are visible, both exhibiting a reddish hue. This red color likely indicates an older stellar population within these nuclei, implying a possible cessation of recent major star formation activity within those regions individually. Faint blue-green light is present in a region that seems to surround both nuclei, suggesting ongoing star formation in the areas connecting the two. Overall, the galaxy lacks well-defined spiral arms or a prominent disk. It presents a smooth and somewhat disturbed morphology, consistent with a system in the late stages of a merger. Tidal features or extended tails are not prominently visible in this image. The system is relatively compact, with the two nuclei situated close to one another.
