The galaxy appears as a moderately luminous object with a redshift indicating a significant distance. Its morphology is predominantly smooth, suggesting an elliptical or lenticular classification. The galaxy exhibits a slight elongation, deviating from a perfectly circular shape. No prominent spiral arms or distinct disk structures are discernible in this image. The color profile indicates a population of older stars, with a relatively low rate of star formation, and a redder overall hue. There is no evidence of ongoing major mergers or significant tidal disturbances in the visual data. The light is centrally concentrated, and a smooth transition to the background sky surrounds the object.
