The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated luminosity profile, with a bright, yellowish core. The light distribution suggests a high degree of spherical symmetry, with a smooth falloff in intensity from the center outwards. There is a slight color gradient, with the core appearing redder than the outer regions, which have a more yellow appearance. This could indicate an older stellar population in the center and relatively younger populations in the outer regions. There is no apparent disk structure, spiral arms, or significant dust lanes visible. Overall, the galaxy appears undisturbed and relatively evolved.
