The galaxy appears to be a relatively smooth, elliptical system at a redshift indicative of a considerable distance. Its morphology is dominated by a central bulge that emits strongly, appearing a yellowish-orange hue. The light gradually fades away from the center in all directions, indicating no strong features such as spiral arms or a prominent disk. The overall shape is roughly circular in projection, displaying only a slight elongation. There is no evidence of ongoing major mergers or tidal disturbances. Based on the color profile, stellar populations are likely aging and the rate of star formation is subdued.
