This galaxy presents as a relatively smooth, centrally concentrated system, exhibiting a high degree of symmetry. Its overall shape is broadly elliptical, appearing mostly round but with a subtle elongation. There is no discernible disk structure or spiral arm morphology. The galaxy's light profile suggests a smooth transition in brightness from a bright core region outward to a less luminous halo. The core region appears slightly redder in color, while the outer halo has a bluer hue. There is no visual evidence of strong tidal features, major mergers, or significant dust lanes within the galaxy. The overall impression is of an evolved galaxy with a well-mixed stellar population and minimal ongoing star formation.
