The galaxy presents a largely smooth morphology, appearing as a moderately elliptical structure. There is a distinct color gradient visible, shifting from a more yellow-white hue in the central region to a redder hue in the surrounding outer regions. This color variation suggests potential differences in stellar populations and/or dust content across the galaxy. A very subtle hint of a possible tidal feature or minor disturbance is faintly discernible along one side of the galaxy, though the data suggests there are no mergers occurring.