The galaxy appears to be a relatively smooth elliptical galaxy, with a highly concentrated central bulge. The light distribution is centrally concentrated, and the overall shape is approximately round. There is little evidence of spiral arms or a distinct disk structure, but there is evidence of some disturbance in the features. The color indices suggest a moderate population of older stars, with possibly an intermediate amount of on-going star formation. It is estimated to be a fairly massive galaxy. The galaxy appears to be relatively isolated with no significant signs of major merger activity.
