This galaxy appears to be a relatively smooth, disk-dominated system, presenting an elliptical morphology. The central region exhibits a brighter, more concentrated light profile that fades outward. There is no apparent bar structure. The disk displays a subtle blue tint, suggesting the presence of younger stellar populations and potentially ongoing star formation activity. There is a very slight hint of distortion present in the outer regions. While no major mergers are apparent, there may be minor disturbances present.
