The galaxy exhibits a relatively compact structure with a disturbed morphology, hinting at potential interaction or recent merger activity. A disk-like component appears present, though its structure is irregular. There's evidence of significant tidal disturbance, potentially indicating ongoing gravitational interaction with another galaxy, or a remnant of a recent merger. A bridge of material could be seen extending from one of the merging galaxies. Overall, it appears to be a dynamic system undergoing significant morphological transformation. Star formation is occurring, but at a lower than average rate for galaxies of similar mass.
