The galaxy appears as a roughly circular, centrally concentrated object, presenting a smooth, largely featureless morphology. There is a hint of disturbed structure or faint tidal features, indicating possible gravitational interaction with another galaxy. The light distribution suggests a relatively even spread across the galaxy, with a gradual decrease in intensity toward the outer regions. The galaxy appears largely round in shape. There is a slight hint of asymmetry in the outer regions. There is also an indication of a minor disturbance, possibly due to a minor merging event.
