The galaxy presents as an elliptical or lenticular type system, exhibiting a smooth and centrally concentrated light distribution. A dominant, relatively bright nucleus is apparent, surrounded by a more diffuse halo of light. The galaxy appears primarily yellow, with some redder areas, suggesting a population of older stars and a low current star formation rate. There is no obvious spiral structure or prominent dust lanes, but a very slight flattening is visible along one axis. The overall morphology suggests a system that is not currently undergoing any major merger activity, but could be interacting with its surroundings.
