The galaxy appears as a relatively compact, smooth object with a dominant central concentration of light. Its overall shape is elliptical or spheroidal, displaying a high degree of circularity with minimal elongation. There is no discernible spiral structure or prominent disk visible. The color gradient suggests a population of evolved stars, with a redder hue dominating the galaxy's light, particularly in the core. There are no indications of major ongoing mergers or significant tidal disturbances; however, there might be some subtle asymmetry suggesting minor interactions or internal dynamics. The galaxy shows a weak bluer tint near the center, suggesting the possibility of ongoing star formation, although at a low rate. The galaxy's small apparent size and high redshift indicate that this is an intrinsically small galaxy, and it is at a considerable distance.
