The galaxy appears as a flattened, elliptical object. A concentrated, bright central bulge is evident, indicative of a high stellar density in the galactic nucleus. The overall color profile suggests an older stellar population, with a yellowish hue dominating the central region. Extending outwards from the core, there's a more diffuse, less luminous halo or disk. The disk presents a bluer color suggesting more active star formation. However, this bluer region is not highly structured or resolved in this image, indicating either a smooth distribution of younger stars or that the star-forming regions are obscured by dust. There's no prominent spiral arm structure visible. The galaxy exhibits a relatively smooth morphology, showing no major disturbances or signs of recent major merger events. There may be evidence of minor disturbance in the galaxy's shape.
