The galaxy presents as a relatively smooth, elliptical structure. The color profile suggests a dominant population of older stars, with a noticeable yellow hue at the galaxy's core, transitioning to slightly redder tones in the outer regions. No distinct spiral arms or prominent dust lanes are visible. The galaxy exhibits a high degree of radial symmetry and appears undisturbed, lacking any apparent signs of tidal interactions or ongoing mergers. The morphology appears largely spheroidal, with a centrally concentrated luminosity profile, and a consistent luminosity gradient.
