The galaxy presents as a centrally concentrated object with a smooth light distribution. It appears largely featureless in this image, lacking prominent spiral arms or a distinct disk structure. The shape is generally rounded, exhibiting minimal elongation. A slight color gradient is observed, with the central region appearing marginally redder compared to the outer regions, suggesting a potentially older stellar population in the galactic nucleus. There is no apparent ongoing major merger activity or significant tidal disturbance evident in the image.
