The galaxy presents as a centrally concentrated object with a largely smooth morphology. A slight elongation is observed, deviating from a perfectly circular form. The primary color is a bright white, suggesting a significant population of hot, young stars or a prominent active galactic nucleus. There is a subtle color gradient outward from the center, transitioning to a more reddish hue in the outer regions. The image suggests minimal signs of major disturbances or ongoing mergers, although some minor irregularities may be present. These could suggest minor interactions or internal structures. Overall, the galaxy appears relatively evolved, with a potentially declining star formation rate indicated by the redder colors in the outer regions, though the central white color indicates relatively high recent or on-going star formation.
