The galaxy presents a somewhat amorphous and disturbed morphology. There appear to be multiple luminous concentrations within the galaxy, suggesting either multiple nuclei or distinct regions of enhanced star formation, possibly indicative of an ongoing merger event. These brighter regions exhibit a yellowish-orange hue, which could point to an older stellar population or significant dust obscuration. Overall, the galaxy does not exhibit a strong disk or spiral structure, but instead has a clumpy and irregular appearance. There also is not a clearly visible galactic center, but the lack of visible features could be attributed to the galaxy's high redshift, which renders fine details more difficult to resolve. Faint tidal features may be present, extending from the main body of the galaxy, supporting the hypothesis of a recent or ongoing merger.
