The galaxy presents as a centrally concentrated, smooth structure with a notable radial gradient in color. The central region displays a pronounced yellow hue, which gradually transitions to a redder color profile at the outer edges of the galactic disk or bulge. There is no discernible spiral arm structure or significant dust lane obscuration visible. The overall morphology suggests a relatively undisturbed system, potentially an elliptical galaxy or a lenticular galaxy seen face-on. The object exhibits a high degree of central concentration. There is no evidence of major ongoing mergers or tidal disturbances. The light distribution appears relatively symmetric, suggesting a lack of significant recent interactions.
