The galaxy presents a primarily smooth morphology, with a generally elliptical shape. There is a high degree of radial symmetry, and the galaxy appears relatively undisturbed, lacking strong indications of recent major mergers or tidal disruptions. The color distribution suggests a centrally concentrated population of older stars. The bluer color component extends further from the core, suggesting a faint disk or other region of on-going star formation activity in the outer regions. The galaxy displays an intermediate ellipticity, appearing neither perfectly spherical nor highly elongated. Overall, the galaxy exhibits characteristics consistent with a relatively evolved system.
