The galaxy presents as a diffuse, luminous structure with a smooth, elliptical morphology. It displays a central concentration of light that fades gradually toward the outer edges. The color gradient suggests a dominant population of older stars, with a general lack of prominent dust lanes or distinct spiral arm structures. The galaxy appears relatively undisturbed, exhibiting a well-defined shape with minimal signs of tidal interactions or ongoing major mergers. It has a slightly elongated shape. There might be some low levels of star formation occurring.
