This galaxy appears to be a relatively smooth elliptical galaxy, characterized by a high degree of central concentration. It exhibits a spheroidal morphology with a moderate ellipticity. There is a noticeable radial color gradient, transitioning from a bright, yellowish core to a dimmer, redder halo region. No distinct spiral arm structures or dust lanes are visible. The galaxy is dominated by older stellar populations, as indicated by the redder overall color. There's no apparent evidence of ongoing major merger activity. The overall structure suggests a mature system with relatively low current star formation.
