The galaxy appears to be an elliptical or lenticular type. The light is concentrated in a smooth, centrally located bulge that dominates the overall structure. There is no apparent spiral arm structure and the galaxy is characterized by a generally featureless morphology. The light emitted by the galaxy appears to be of a slightly yellowish or reddish hue. This suggests that the galaxy is primarily populated by older stars. The galaxy's shape is somewhat elongated, showing a moderate ellipticity. There are no obvious signs of recent or ongoing major merger events. There is no visible dust lane and the morphology suggests the rate of star formation may be relatively low.
