The galaxy exhibits a merging morphology. It shows a disturbed structure, indicating an interaction with another galaxy. There appears to be two distinct nuclei, suggesting the late stages of a merger. The color appears redder, which could indicate an older stellar population and suppressed star formation within the galaxy. The galaxy appears to have a relatively smooth appearance, with no well-defined spiral arms or significant dust lanes visible. The overall shape is moderately elliptical, as opposed to a clear disk or spherical structure.
