The galaxy presents an overall elliptical morphology, appearing relatively smooth in structure. A bright, concentrated central bulge dominates the light profile, indicating a high concentration of stars in the nucleus. Surrounding the bulge is a fainter, more diffuse halo of stars, which is slightly elongated. The color gradient suggests older stellar populations. No distinct spiral arm structures or prominent dust lanes are visible, supporting its classification as an elliptical galaxy. There may be a minor disturbance in the structure.
