The galaxy presents as a centrally concentrated object with a generally smooth, elliptical morphology. It exhibits a color gradient, appearing more yellow/orange toward the core, suggesting a dominant population of older stars in the central bulge. There are some signs of disturbed morphology, with potential asymmetries or faint tidal features hinted at in the surrounding diffuse light, though these are very subtle. The overall roundness of the galaxy suggests it is likely an elliptical galaxy with a relatively low star formation rate, and it shows no obvious signs of a spiral disk or strong ongoing mergers. The moderate redshift value indicates that this galaxy is at a significant distance from us.
