The galaxy presents as a relatively compact object. Its central region exhibits a high surface brightness, appearing nearly unresolved and intensely luminous. A faint, diffuse halo surrounds this central core, showing a gradual decrease in luminosity with increasing radial distance. The morphology appears largely smooth. Subtle color variations are discernible within the diffuse halo, indicating potential variations in stellar populations. The overall symmetry suggests a lack of major disturbances or ongoing merger activity, though slight asymmetries in the outer regions cannot be entirely ruled out. The galaxy appears primarily spheroidal.
