The galaxy presents as a system undergoing a significant interaction. The primary body of the galaxy is somewhat elongated, with a suggestion of a distorted disk. It shows a smooth appearance, lacking strong spiral arm definition. There is a noticeable extension or tidal tail emanating from one side of the primary galaxy, suggesting gravitational disruption.

There appear to be multiple distinct, compact bright knots or cores within the galactic structure. These features exhibit a higher concentration of light and may indicate regions of enhanced star formation triggered by the interaction. The color distribution is not uniform across the galaxy, indicating varying stellar populations or dust content. The presence of bluer hues in some regions suggests ongoing star formation, while redder hues in others could indicate older stellar populations or dust obscuration.
