The galaxy presents as a somewhat elliptical, centrally concentrated object. The core exhibits a bright, yellow-white luminosity, suggesting a significant population of older stars. The galaxy shows a smooth light distribution with a near lack of discernible spiral arm structures or irregular features. The smooth texture indicates that it is a relatively undisturbed system with no major merging events or strong tidal interactions apparent. There is a subtle color gradient from the core outwards, with the outer regions appearing marginally redder. This color shift could indicate a variation in stellar population age or metallicity. The galaxy does not show evidence of active star formation, based on the lack of blueish or irregular structures, but may host a population of low-level star formation activity. The general morphology suggests an elliptical or lenticular galaxy type.
