The galaxy appears to be a merging system, potentially consisting of two distinct galactic nuclei or high-density regions. The primary component exhibits a yellowish-white core, indicating a possible concentration of older stellar populations. A subtle redder hue surrounds this core on one side, which might be indicative of dust absorption or a region of enhanced star formation behind the visible core. The second component is less defined, appearing as a fainter, elongated cloud. There is visible distortion in the overall morphology of the combined object. The combined object shows significant luminosity, suggesting the presence of a substantial stellar population. The object's colour profile across g, r, and z bands suggests high mass and low specific star formation rate.
