The galaxy presents as a largely smooth, centrally concentrated object. The galaxy exhibits a near circular morphology, with a slight elongation. There is minimal evidence of spiral arm structure or pronounced disk features. Color gradients suggest a possible radial variation in stellar populations or dust content. The galaxy has a moderately bright core that fades smoothly to its edges. There appears to be a faint extension or a very minor disturbance in the main body of the galaxy. The galaxy appears to be a relatively undisturbed system.
