The galaxy appears as a centrally concentrated object with a smooth, diffuse morphology. Its shape is roughly round, displaying only a minor deviation from perfect circularity. The central region exhibits a bright, concentrated core, suggesting a high density of stars or potentially an active galactic nucleus, although no distinct features are resolved at this resolution. The galaxy’s light profile fades gradually from the center outwards, with no apparent spiral arms or distinct disk structure. Color gradients across the galaxy suggest variations in stellar populations, the central bulge appearing more yellow or golden in color compared to the outer regions which appear more white and blue. There is no obvious evidence of recent major mergers or significant tidal disturbances in this image; its overall structure indicates it is relatively undisturbed. However, there seems to be a redder halo, possibly indicating older stars.
