The galaxy appears to be undergoing a significant interaction, possibly a merger. There are noticeable tidal features or distortions indicating gravitational disturbances. The central region exhibits a relatively smooth, concentrated morphology, with a yellowish hue suggestive of an older stellar population. Two distinct bright nodes are present, one with a reddish tint, indicating possibly active star forming regions or a strong H-alpha emission. The overall color gradient suggests variations in stellar populations and dust content across the galaxy. The system does not exhibit a clear spiral structure. A fainter tail extends outwards, likely formed by material stripped during the interaction, but that may be a merging galaxy itself.
