The galaxy presents as a relatively smooth, concentrated object. Its morphology appears elliptical, with a high degree of central concentration that fades outwards. The core exhibits a yellowish hue, suggesting an older stellar population. Moving outwards, the galaxy transitions to a bluish-white color, implying the presence of younger stars in the outer regions, or possibly ongoing, albeit low, star formation. There's a subtle suggestion of a disk structure. There's no discernible evidence of major mergers or tidal disturbances in this image.
