The galaxy presents as a centrally concentrated, relatively smooth object. It appears elliptical in shape, with a high degree of rotational symmetry. The core exhibits a strong yellow hue, suggesting a higher concentration of older stellar populations and potentially a more significant dust component. Moving outward from the core, the color transitions gradually to a faint greenish yellow halo. There is very little evidence of well-defined spiral arm structures, with only a hint of possible disk features. The galaxy does not seem to show any signs of major disturbances or ongoing mergers. The overall morphology points to a galaxy that has largely completed its star formation, or whose star formation rate is currently low.
