The galaxy presents as a relatively smooth, elliptical-like structure. The core region exhibits a concentrated luminosity, appearing a bright yellow-white. This suggests a significant population of older stars. A diffuse, greenish-blue halo surrounds the core, possibly indicating a more extended distribution of stellar populations or ionized gas. There is no obvious spiral arm structure or significant dust lane obscuration visible. The overall morphology suggests a galaxy that is not currently undergoing a major merging event, with a relatively regular and relaxed appearance.
