The galaxy presents as a centrally concentrated object with a smooth, diffuse halo extending outwards. The core exhibits a bright, yellowish hue, suggesting an older stellar population. The halo appears fainter and slightly bluer, which may indicate the presence of younger stars or recent star formation in the outer regions. Overall, the galaxy's morphology suggests an elliptical or lenticular type with a relatively high Sersic index, indicating a steep brightness gradient towards the center. The ellipticity is moderate, showing that the galaxy is somewhat flattened but not highly elongated. There is no clear evidence of spiral arms or a prominent disk structure based on the image alone.
