The galaxy exhibits a distinct morphology suggesting an ongoing interaction or recent merger. The primary body of the galaxy appears elongated and somewhat disrupted, showing a possible tidal tail or stream extending from one end. A secondary, smaller, and more compact component is observed near the primary body, potentially indicating a merging dwarf galaxy or a region of intense star formation triggered by the interaction. The color of the galaxy is primarily reddish, suggesting an older stellar population and/or significant dust obscuration. There is a possibility for presence of active galactic nucleus, but it requires further spectra analysis.
