The galaxy presents as a complex morphological structure, exhibiting characteristics suggestive of an ongoing or recent merger event. Multiple luminous components are visible, with varying degrees of connectivity. A central, moderately bright, diffuse region appears yellowish, potentially indicating an older stellar population. An adjacent, slightly redder and more compact region is present, possibly representing a distinct galactic nucleus or a region of intense star formation obscured by dust.

Extending from the central region are fainter, elongated features, some appearing fragmented. These could be tidal tails formed through gravitational interactions. A portion of the galaxy displays a bluer hue suggesting the presence of younger stars and ongoing star formation. Overall, the morphology is disturbed and irregular, indicative of a dynamic system undergoing significant gravitational interactions and star formation activity, with a mass upwards of 10^11 solar masses. It is located at a redshift of approximately 0.228, corresponding to a significant distance.
