The galaxy presents a generally smooth, elliptical morphology. The light distribution is centrally concentrated with a gradual decrease in surface brightness moving outward from the core. There is a slight elongation visible, hinting at a deviation from a perfect spherical shape. A subtle disklike structure may be present that is slightly offset from the center. The galaxy exhibits a color gradient, with the central region appearing more yellowish-white. Fainter, bluer light can be seen in the outer regions of the galaxy, implying a difference in the stellar population. The galaxy does not show any signs of major disturbances or ongoing mergers, although some very faint irregularities are present.
