The galaxy presents as a merging system, with at least three discernible components. The dominant feature is a yellowish, centrally condensed region, suggesting a significant concentration of older stellar populations. A fainter, somewhat elongated component is observed to the upper left of this central region, displaying a slightly reddish hue. To the upper right, another component is noted, appearing more compact and with a bluer color, possibly indicating younger stars or active star formation. The overall morphology suggests ongoing gravitational interaction and disruption, characteristic of a merger event. The galaxy has an estimated size of approximately 7 kiloparsecs, and has a relatively high mass, likely exceeding 10^11 solar masses. The measured redshift places it at a considerable distance. Estimated absolute magnitudes are relatively bright, likely due to relatively low, but not insignificant, star formation rates. The estimated specific star formation rate is relatively low, suggesting this galaxy has not been actively forming stars recently. Overall, the visual impression supports a system where the effects of merging are still apparent, and the final morphology of the merged galaxy has not yet stabilized.
