The galaxy presents a largely smooth, elliptical morphology. There is a high degree of central concentration with a bright core that diminishes in intensity outwards. The radial color profile suggests the presence of older stellar populations, with a yellowish central bulge. The overall structure exhibits a high degree of symmetry, lacking any obvious signs of significant tidal disturbances or ongoing major mergers. Subtle irregularities are possibly present in the outer regions, but their prominence is very low. No distinct spiral arms or a well-defined disk component are discernible. The galaxy appears relatively isolated, with no clear indications of close companion galaxies or significant interactions.
