The galaxy presents as a generally smooth, elliptical or spheroidal structure. The central region exhibits a high degree of luminosity, appearing bright yellow, indicating a significant concentration of older stellar populations. There is a subtle color gradient extending outward from the center, with the outer regions appearing less luminous. There is no distinct spiral arm structure or prominent dust lanes visible, reinforcing the elliptical/spheroidal morphology. There is no evidence of a major ongoing merger, although minor irregularities in the outer regions cannot be definitively ruled out at this resolution. Overall, the galaxy is round in appearance and has a low star formation rate.
