The target galaxy presents as a system exhibiting evidence of an ongoing or recent merger event. The primary body displays a disturbed morphology, lacking a well-defined spiral arm structure or elliptical shape. There are multiple concentrations of luminosity within the galaxy, suggesting the presence of interacting or recently merged galactic nuclei. The distribution of light is not uniform, indicating regions of enhanced star formation or tidal debris resulting from the interaction. The overall color of the galaxy appears relatively blue, potentially indicative of a younger stellar population and active star formation. The system is elongated, possibly a consequence of the gravitational interactions. Evidence of tidal tails or bridges extending from the galaxy is not distinctly visible in this image, although the diffuse and irregular shape hints at such features. Based on this, this system may be classified as a late-stage merger remnant.
