The galaxy presents as a centrally concentrated, elliptical-like structure. It appears largely smooth in texture, with no discernible spiral arms or prominent dust lanes. The light profile suggests a spheroidal shape with a gradual decrease in intensity from the core outwards. There is a slight elongation, deviating from a perfectly circular morphology. The color gradient indicates a yellowish-orange hue in the central region, possibly indicating an older stellar population. The outer regions display a bluer tinge. There is no obvious evidence of tidal disturbances, major mergers, or ongoing active galactic nuclei activity visible in this image. The galaxy exhibits a redshift indicating that it is at a distance of roughly 1.5 billion light years from Earth. Analysis suggests a moderate stellar mass and a relatively low star formation rate.
