The galaxy presents as an elliptical morphology with a high degree of central concentration. Its color profile suggests a predominantly older stellar population, as indicated by the yellow to red hues. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy appears relatively smooth in texture, lacking obvious signs of recent major mergers or significant tidal disturbances. There may be minimal star formation activity. The round shape suggests that we are viewing the galaxy close to face-on.
