The galaxy presents as a relatively smooth, elliptical morphology. The light distribution appears centrally concentrated, exhibiting a gradual decrease in brightness towards the outer regions. There is a slight elongation in the galaxy's shape, although it is generally round. Based on its appearance, the galaxy appears to be a relatively undisturbed system. The color gradient suggests a higher concentration of older stellar populations, indicated by the redder hue in the galaxy's core. There does not appear to be substantial evidence of spiral arm structures or significant dust lanes.
