This galaxy presents as a relatively smooth, elliptical object. The galaxy exhibits a concentrated central bulge that is approximately 7 kiloparsecs in radius. The morphology shows a preference towards being an elliptical galaxy. The light from this galaxy appears to be more concentrated towards the redder wavelengths. This possibly signifies an older stellar population. There appears to be a slight disturbance, possibly indicative of a minor interaction with another galaxy or past accretion event. There is no apparent ongoing major merging event.
