The galaxy presents a generally smooth morphology with some features that suggest possible disturbance. The central region appears bright and relatively featureless, with a slightly elongated shape. A faint tidal tail extends from the central region, displaying a gradient of colors from bluish-green closer to the center, transitioning to a reddish hue at its extreme extent. The overall color of the galaxy appears somewhat redder than typical spiral galaxies, and there is evidence of ongoing or recent star formation activity as indicated by the bluer regions near the tail. Morphological analysis indicates a higher probability of a smooth structure but some possibility of disturbances.
