This galaxy appears to be an elliptical type, observed at a redshift suggesting a significant distance. The morphology is predominantly smooth, showing little evidence of spiral arms or significant dust lanes. The central region exhibits a higher concentration of light, appearing yellowish, possibly indicating an older stellar population. Fainter, bluer light extends outward from the core, suggesting recent or ongoing star formation activity, though subdued. The galaxy's shape is elongated, approximating a cigar shape, with no strong evidence of recent major mergers or tidal disturbances.
