The galaxy presents as a centrally concentrated object, likely an elliptical or lenticular type. It exhibits a smooth, diffuse light distribution, with minimal discernible substructure such as spiral arms or prominent dust lanes. The color profile suggests an older stellar population, indicated by the yellowish-orange hue concentrated in the core. The galaxy has a nearly circular morphology. There is a slight color gradient observed from the center outwards, with a subtly bluer halo surrounding the yellower core, potentially indicating ongoing, but low levels of star formation in the outer regions. There is no obvious evidence of tidal disturbances or ongoing mergers based on the morphology.
