The observed galaxy appears to be undergoing a significant interaction or merging process. There are two distinct, bright cores evident, suggestive of two galactic nuclei in close proximity. The overall shape is irregular and elongated, not displaying a clear spiral or elliptical structure. The color gradient transitions from a yellowish hue in the central regions, indicating older stellar populations, to a bluer tint in the outer regions, potentially indicating the presence of some star formation. There are faint tidal features or tails extending from the main body, suggesting gravitational disruption. Overall, the morphology indicates a galaxy experiencing an advanced stage of merging activity with potential tidal disturbances.
