The galaxy presents as a luminous, centrally concentrated object. Its morphology appears relatively smooth and elliptical in shape with no obvious spiral arm structures. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population. The intensity of color decreases towards the outer edges, fading into a slightly redder shade, implying some degree of color variation in its stellar components. There are no strong indications of tidal disturbances or ongoing major mergers, as the structure looks fairly undisturbed. There is a subtle, very diffuse halo of material extending outwards from the main body of the galaxy.
