The galaxy presents a largely smooth morphology, exhibiting a centrally concentrated structure with a radial decrease in luminosity. The overall shape appears elliptical, displaying a high degree of roundness. The central region is dominated by a bright, concentrated core. There is no apparent spiral arm structure or evidence of a significant galactic disk. Faint extensions surround the core. There are no clear indications of ongoing major mergers or significant tidal disturbances. The color profile suggests a population of older stars.