The galaxy appears to be undergoing a significant interaction, possibly a merger event. There is a bright, relatively concentrated core region exhibiting a slightly pinkish hue, suggesting a population of younger stars or potential active galactic nucleus activity. Emanating from this core, there is a prominent tidal tail extending outwards. The tidal tail displays a yellowish-orange color, which could be indicative of an older stellar population within the disrupted structure. This tail exhibits a less defined structure compared to the central core. There is no clear spiral structure or distinct disk component visible. The overall morphology suggests a system dominated by smooth, featureless components with an apparent disturbance caused by the interaction or merger.
