The galaxy presents as a single, relatively smooth object, dominated by light in the redder bands of the spectrum. This suggests a significant population of older stars. There is a subtle, flattened structure in the central region, however the light is centrally concentrated. It would appear that the central region has a small amount of relatively recent star formation. A very high probability exists that this object is undisturbed by a recent merger or tidal interaction. Given the galaxy's overall appearance, it is likely to be a massive system.
