The galaxy presents a morphology suggestive of a system undergoing a merger. The primary body exhibits a relatively smooth, rounded appearance, indicative of an elliptical galaxy or the bulge of a spiral galaxy. A secondary, less defined structure appears closely associated with the primary body, exhibiting a bluer hue, possibly indicating a younger stellar population and ongoing star formation. Tidal features are present, exhibiting an asymmetric disruption of the galaxy's overall structure. The color gradient across the system suggests varying stellar populations, with older, redder stars concentrated in the primary body, and younger, bluer stars forming in the interacting region. Overall, the system demonstrates characteristics of a dynamic interaction between two galaxies, with ongoing star formation likely induced by the merger event.
