This galaxy exhibits a largely smooth morphology, appearing nearly elliptical in shape. There is a slight elongation, but it is mostly rounded. The central region shows a higher concentration of light, indicative of a bulge. The galaxy displays a color gradient, transitioning from a bluer hue in the core to more red in the outer regions. The smoothness suggests an older stellar population with minimal ongoing star formation, with an estimated mass of around 10^10 solar masses. There are no obvious signs of tidal disturbances or interactions with other galaxies, suggesting it is not currently undergoing a major merger event. Some minor disturbances are possible. The galaxy is relatively compact, with an estimated effective radius of about 5.7 kpc. At its redshift, it is a luminous object in the observed optical bands.
