The galaxy presents as a smooth, elliptical-like object with a concentrated central bulge. The light profile exhibits a radial gradient, transitioning from a bright, yellowish core to fainter, reddish outskirts. There is a subtle suggestion of a flattened, disk-like component extending from the central region, but the overall morphology appears dominated by a spheroidal structure. The color indices suggest a population of older stars, particularly in the outer regions, while the core shows some signatures of more recent, albeit subdued, star formation. There is no evidence of prominent spiral arms, bars, or significant dust lanes. The overall form appears relatively undisturbed with no obvious signs of ongoing mergers or tidal interactions. The axial ratio indicates a moderate ellipticity, exhibiting a shape that is neither perfectly spherical nor highly elongated.
