The galaxy appears as a diffuse, centrally concentrated object with an overall elliptical morphology. The central region exhibits a yellowish-white hue, suggesting an older stellar population. The outer regions are fainter and display a slightly bluer tint, indicative of more recent star formation. There are hints of subtle disturbances in the galaxy's morphology, particularly in the form of faint, irregular extensions or tidal features. The galaxy does not exhibit prominent spiral arms. Its structure appears mostly smooth, but it does show some signs of being a disturbed system, possibly undergoing a minor merger event.