The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. It exhibits a nearly circular appearance. There is little evidence of spiral arms or prominent disk features. The color profile suggests a population dominated by older stars, appearing redder, with possible star formation activity occurring within the central region, presenting a relatively bluer color. The galaxy shows no obvious signs of major mergers or significant tidal disturbances. The overall structure indicates a relatively evolved system.
