The galaxy presents as a smooth, centrally concentrated object. Its morphology appears largely elliptical, with a high degree of circularity. The light profile is diffuse and lacks any discernible spiral arm structures or prominent features indicative of ongoing star formation. The color is predominantly yellow-red, suggesting a population of older stars and a relative dearth of young, blue stars and nebulae. There is no apparent evidence of significant tidal disturbances or ongoing mergers with other galaxies.
