The galaxy presents a smooth, elliptical morphology with a noticeable central bulge. It exhibits an intermediate ellipticity, appearing neither perfectly spherical nor highly elongated. The light distribution suggests a relatively uniform stellar population, though a slight color gradient is observed, trending towards bluer hues at the outer edges of the visible structure and more red toward the core. There is no obvious evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, showing no strong indications of ongoing major mergers or tidal interactions. The light is concentrated in the center of the galaxy, and the galaxy is likely quite massive.
