The galaxy presents as a moderately luminous object with a complex morphology. It appears to be undergoing a significant interaction or merging event. A dominant, roughly spherical component, potentially the remnant core of a progenitor galaxy, exhibits a yellowish hue, suggestive of an older stellar population. Fainter, reddish structures are visible, indicating regions of potentially ongoing or recent star formation. The overall shape is irregular and disturbed, lacking a well-defined spiral or elliptical structure. Based on the disrupted morphology and the presence of multiple components, this system may be in the advanced stages of a galactic merger, likely to evolve into an elliptical or irregular galaxy over time.
