The galaxy presents a largely smooth morphology, with a dominant, concentrated central bulge. The light profile appears largely elliptical, showing a high degree of rotational symmetry, with no apparent disk structure or spiral arms. The color gradient suggests a population of older stars, potentially with ongoing, but low levels of star formation, possibly confined to the central region, given the more yellow color. There is no strong evidence of tidal disturbances or mergers. Overall, based on the image, it appears to be a giant elliptical galaxy. 
