The galaxy presents a generally smooth, elliptical morphology, exhibiting a high degree of radial symmetry. The central region is characterized by a bright, concentrated core that gradually decreases in luminosity towards the outer edges. The overall color profile suggests a population of older stars with a subtle red-shifted hue. There appears to be minimal evidence of spiral arm structure, active star formation, or dust lanes within the visible spectrum. The galaxy is largely undisturbed, lacking any signs of major mergers or tidal distortions. The structure appears to be a single, spheroidal component without any obvious secondary structures or companions.
