The galaxy appears as a singular, relatively undisturbed, and generally smooth object. Its morphology is largely elliptical. A degree of roundness is evident in its overall shape. The galaxy exhibits a central concentration of luminosity, with intensity gently diminishing towards its edges. Colors observed across the galaxy are distributed in such a way that the central region appears slightly more yellow/orange than the outskirts, which trend towards a bluer hue. This could be attributed to differences in stellar populations, dust extinction, or varying levels of star formation between the core and outer regions of the galaxy. There seems to be a central bulge. Based on its appearance, it is likely a relatively massive galaxy with a moderate star formation rate, and a redshift suggesting its light has travelled a considerable distance.
