The galaxy presents as a moderately bright, elliptical structure. Its core exhibits a concentrated luminosity, displaying a yellowish-white hue suggesting a population of older stars. Progressing outwards from the core, the galactic profile gradually diffuses into a less intense halo. The halo is composed of fainter, redder light, potentially indicating a diminishing density of older stellar populations and a lower rate of star formation. The overall shape is somewhat oblate, appearing more rounded than elongated. No distinct spiral arm structures or significant dust lane features are discernible. Minimal signs of recent or ongoing merger activity or morphological disturbance are present. The galaxy appears relatively quiescent.
