The galaxy presents as a system undergoing a significant interaction, possibly a merger. The primary structure exhibits a distorted morphology, appearing elongated and stretched, suggesting tidal forces are at play. A secondary, more compact concentration of light is observed at one end, possibly the remnant core of a merging galaxy or a region of intense star formation triggered by the interaction. The color gradient suggests a population of older stars dominating the overall light, with hints of younger, bluer stars in localized regions. There are observable disturbances, potentially including faint tidal tails or bridges extending from the main body. The relative smoothness indicates a partially completed merging process, where much of the initial structure has been disrupted, but a final equilibrium has not yet been reached.
