The galaxy presents as an elliptical morphology, appearing somewhat flattened but largely smooth in texture. A central bulge region exhibits a concentrated, yellow-orange hue indicative of an older stellar population. Surrounding the bulge, a more diffuse halo extends outwards, displaying a bluer tinge suggesting the presence of some younger stars. The overall structure shows a moderate degree of uniformity, with only subtle irregularities apparent, perhaps indicative of minor past interactions or disturbances.
