The galaxy presents as a system undergoing a significant interaction or merger. The overall morphology is disturbed and asymmetric.

A central, bright region, likely a galactic nucleus, is visible with a somewhat indistinct yellow hue. Surrounding this core, diffuse and irregular structures extend outwards, indicative of tidal features. A long tail-like structure extends from the core, suggesting a gravitational disruption event. The color of this tail looks to be on the bluer side.

There is little evidence of well-defined spiral arms or a regular disk structure. Overall, the galaxy displays characteristics consistent with a major merger event disrupting its original morphology and potentially triggering star formation.
