The galaxy appears as a centrally concentrated object, exhibiting a smooth morphology with a subtle elongation. The core displays a yellow-orange hue, suggesting an older stellar population or significant dust obscuration. The outer regions appear fainter and somewhat redder than the core, consistent with the presence of older stars. There appears to be no distinct disk structure or spiral arms evident in this image, with the overall shape being somewhat elliptical. There are no signs of recent major merger activity, but subtle irregularities may point to minor gravitational interactions in the past.
