The galaxy appears to be in the process of merging or undergoing a significant gravitational interaction. It exhibits an asymmetrical morphology, displaying two distinct nuclei with differing color profiles. The primary nucleus presents a yellow-orange hue, suggestive of an older stellar population. The secondary nucleus appears bluer in color, potentially indicating ongoing star formation. The overall structure exhibits a degree of smoothness, but distortions are apparent, possibly due to tidal forces from the interaction. These disturbances are visible as faint, diffuse extensions from the main body of the galaxy. The galaxy's shape can be described as generally round in form, but with noticeable deviations.
