The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a slight elongation, appearing somewhere between round and cigar-shaped. There is no prominent disk structure visible, nor any signs of major disturbances or ongoing mergers. The light is yellowish-white, with a more diffuse and slightly bluer halo surrounding a brighter, more concentrated central region. This may indicate a population of older stars dominating the central region, with a more recent, albeit weak, star formation occurring in the outer regions. The relatively smooth morphology suggests a galaxy that has largely completed its major assembly and is evolving relatively passively.
