The galaxy presents as a relatively smooth, elliptical form with a moderately concentrated central bulge. Color gradients suggest potential variations in stellar population and age across the galactic structure. The central bulge exhibits a warmer, yellower hue, possibly indicating a population of older, redder stars. Moving outward from the core, the galaxy displays a subtle transition to a cooler, greenish color. This may signify ongoing star formation within a disk-like structure embedded within the elliptical galaxy, or perhaps the presence of younger stellar populations. Overall, the galaxy appears to be a relatively isolated system without strong evidence of tidal interactions or major disturbances.
