The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. The core exhibits a yellowish-white hue, indicating a population of older stars. Extending outward from the core, the galaxy displays a fainter, diffuse halo, which is bluer in color. No distinct spiral arm structures or prominent dust lanes are discernible within the galaxy’s structure. The galaxy shows no obvious signs of major tidal disturbances or ongoing mergers with other galaxies. It appears undisturbed. The overall shape tends towards a round morphology.
