The observed galaxy presents an elongated morphology, with an estimated apparent size of approximately 5.6 arcseconds. The galaxy exhibits a tri-modal color distribution: a centrally located blue region, a yellowish region nearby, and a fainter, redder tail extending asymmetrically. This morphology could indicate a late stage merger event. The blue color suggests a region of active star formation, while the yellow color could be suggestive of an older stellar population. The redder tail exhibits a more diffuse, fainter structure, possibly comprised of stripped material from the main galaxy. There is some evidence of a faint tidal tail-like structure extending from the central body, suggesting gravitational interaction with another galaxy or recent disruption. Overall, the galaxy appears to be experiencing a period of significant morphological and star formation activity, likely driven by an ongoing or recent merger event.
