The galaxy presents as a relatively compact, elliptical morphology. Its light distribution appears smooth and concentrated towards the center, with a gradual decrease in luminosity as we move towards the outer edges. The galaxy exhibits a yellowish hue, indicative of an older stellar population, as expected at its measured redshift. There is no apparent disk structure or spiral arm features visible, although the resolution is limited. There are no signs of tidal tails or major disturbances in the surrounding area, suggesting it has not experienced any recent major mergers or interactions. The object appears to be somewhat isolated in its immediate environment.
