The galaxy appears to be undergoing a merger or interaction. There are two prominent, concentrated regions of light, which could represent the cores of the merging galaxies. The overall structure shows some distortion, lacking a clear, well-defined spiral or elliptical shape. Diffuse, faint light surrounds the brighter regions, indicating tidal debris or extended stellar populations resulting from the interaction. The color distribution seems relatively uniform, with a predominantly yellowish hue in the central regions. This suggests an older stellar population, though there might be some ongoing star formation hinted by slightly bluer regions embedded within the diffused areas. The object displays a moderate degree of roundness, though the interaction gives it an irregular appearance. The morphology is complex, with the possibility of tidal tails or bridges too faint to be clearly distinguished in this image.
