The galaxy appears as a centrally concentrated object with a smooth morphology. It is roughly elliptical, appearing slightly more elongated than perfectly circular. The color profile shows a strong red component, with a hint of green and perhaps a slight touch of blue, concentrated towards the central region. The overall structure suggests a relatively quiescent system. There's no visible evidence of strong spiral arms or active star formation regions within the resolution of this image, implying a more evolved or passively evolving galaxy. The red color suggests a population of older stars is dominant, with possibly low ongoing star formation activity. No significant tidal features or signs of recent major mergers are apparent. There may be minor disturbances. The overall light distribution decreases smoothly from the central region outwards, further supporting a general lack of significant substructure within the galaxy.
