The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. There is little to no visible evidence of spiral arms or a distinct disk structure. The light distribution appears relatively uniform, lacking strong features such as prominent dust lanes or star-forming regions. The overall shape appears nearly circular. There's minimal visible disturbance to the galaxy’s structure. The galaxy exhibits a faint bluish hue, suggesting the presence of some younger stellar populations, although redder tones dominate.
