The galaxy presents a largely smooth, elliptical morphology. It appears centrally concentrated with a bright, yellow-tinged core that gradually diffuses outwards into a fainter halo. The shape is approximately round. There is no immediately apparent spiral structure or distinct dust lanes. No indications of significant tidal disturbances or ongoing mergers are seen. The color profile suggests a population of older stars, typical of elliptical galaxies, with less recent star formation.
