The galaxy presents as a concentrated, elliptical structure with a high degree of central luminosity. The core exhibits a yellow to golden hue, suggesting a population of older stars. Moving outward from the nucleus, the color gradually shifts toward a slightly bluer tone, possibly indicating a region with some ongoing star formation. The overall morphology appears relatively smooth, lacking prominent spiral arms or significant dust lanes. There may be minor tidal disturbance present. The galaxy exhibits a round to slightly elliptical morphology. There is no evidence of a major merger event. Based on its redshift, this galaxy is observed at a considerable distance. The galaxy seems fairly massive, with a moderate amount of star formation.
