The galaxy presents as a relatively smooth, centrally concentrated structure. It exhibits a spheroidal morphology, with a high degree of radial symmetry. The light distribution suggests a dominant bulge component, appearing quite round. The central region is significantly brighter and has a yellowish hue. There is a subtle decrease in light intensity as one moves outwards from the core, transitioning to an extended, fainter halo. Subtle asymmetry is observed in the outer regions, potentially indicating minor tidal disturbances or interactions. Star formation appears to be generally low.
