This galaxy exhibits a generally smooth morphology. It is elliptical in shape, with a high degree of central concentration. The light profile suggests a relatively old stellar population, with a blue hue, implying the presence of ongoing, moderate star formation. There is a slight hint of asymmetry or possible disturbance in the outer regions, although no clear tidal features or obvious signs of a major merger are apparent. The galaxy displays a gradual decrease in luminosity from the center outwards, and no distinctive features such as strong spiral arms, or a prominent bar are visible.
