The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high degree of concentration, appearing as a bright, yellowish-white core. Moving outward from the core, the luminosity gradually decreases, transitioning to a more diffuse, reddish-orange halo. There is a slight elongation, suggesting a deviation from a perfectly spherical shape, appearing more as an oblate spheroid. No distinct spiral arm structures or prominent dust lanes are discernible. The overall color profile indicates a population of older stars, with a relatively low rate of on-going star formation activity. There might be minor disturbances occurring, but there are no signs of major interactions with other galaxies.
