The galaxy appears to be undergoing a major merger. The central region exhibits a somewhat diffuse, though concentrated, light profile, suggesting the presence of an older stellar population. Evident across the body of the galaxy are features characteristic of significant tidal disturbances. These include extended, irregular structures and asymmetries, which are indicative of interactions with another galaxy. Bluer regions are scattered throughout, hinting at ongoing or recent star formation activity. Overall, the galaxy's morphology is far from relaxed, suggesting it's in a dynamically active state.
