The galaxy presents as a generally smooth, elliptical morphology with a centrally concentrated light profile. The core exhibits a yellowish-orange hue, which may indicate an older stellar population. Moving outwards from the core, the galaxy shows a subtle transition to a more greenish color, indicating a possible presence of younger stars than those concentrated in the nucleus. The galaxy appears to be relatively undisturbed, lacking significant signs of tidal features or major merger activity. The overall shape appears slightly elongated. There is a hint of what might be minor structural distortion on one side, but it's difficult to determine at this resolution if that is genuine or noise.
