This galaxy appears to be undergoing a merger or tidal interaction. There is evidence of significant morphological disturbance, with no clear spiral arm structure or elliptical symmetry. One distinct, compact region with a yellowish color is visible on one side of the galaxy. The main body shows a more diffuse, irregular shape with a predominantly blue color. This may indicate ongoing or recent star formation within this region. The overall light distribution is clumpy rather than smooth, suggesting that this galaxy is not relaxed and could be undergoing significant gravitational interaction. The object has an estimated size of a few kiloparsecs. Further analysis is required to determine the details of the interaction and the specific properties of the stellar populations within each region.
