The galaxy appears to be relatively smooth and elliptical in shape, exhibiting a high degree of radial symmetry. It lacks prominent spiral arms or a well-defined disk structure. The central region of the galaxy shows a concentration of light, suggesting the presence of a dense galactic nucleus or bulge. The color gradient across the galaxy appears subtle, with a slightly redder hue in the central region and a bluer tinge in the outer regions, potentially indicating differences in stellar populations or dust content. There is no clear evidence of major ongoing mergers or tidal disturbances.
