This galaxy appears as a relatively compact, elliptical-like object with a smooth overall structure. Its color profile suggests a dominance of older stellar populations, exhibiting a yellowish-orange hue. There is no discernible spiral arm structure or prominent dust lanes. The galaxy seems to have a high degree of roundness, showing minimal elongation. Subtle indications of minor disturbances may be present, but it does not appear to be undergoing a major merging event. The galaxy's measured redshift places it at a considerable distance. Although not directly visible in this image, its inferred stellar mass is very high. The estimated star formation rate is relatively low indicating it may be quiescent or passively evolving.
