The galaxy presents a generally smooth, rounded morphology. The central region exhibits a bright, concentrated core, possibly indicating a bulge component. Colors are generally redder in the core and become slightly bluer towards the outer regions. There may be some indications of a disk, though this appears faint. There are no obvious signs of major mergers or tidal disturbances. Based on these characteristics, this galaxy might be classified as an early-type spiral or an elliptical galaxy. The redder colors in the core suggests an older stellar population, whereas bluer colors in outer regions suggest younger star formation. Overall the light is evenly distributed across the galaxy.