The galaxy presents as a largely smooth, elliptical form. A central, concentrated bulge is visible, appearing slightly more yellow in hue, suggesting an older stellar population. There is little evidence of spiral arm structure, but the overall light distribution indicates a centrally dominant system. The outer regions appear more diffuse and slightly bluer, potentially indicating a younger stellar population or some ongoing star formation at the periphery, albeit limited. There is no strong indication of major mergers or significant tidal disturbances.
