The galaxy presents as a somewhat diffuse, irregular structure. A relatively smooth, centrally concentrated component is visible, but the overall morphology suggests the presence of features or irregularities, possibly disk-like in nature. There may be some interaction occurring within the galaxy. The color profile is generally blue, suggesting some younger population of stars, but there is a reddish central component, indicating an older population. There is no clear evidence for any major ongoing merger event in this particular image, although there could be a potential minor disturbance. The estimated size would classify it as a relatively small galaxy.
