The galaxy appears as a single, concentrated, centrally-brightened object. The light distribution is smooth and elliptical with high degree of central symmetry. The morphology is dominated by its spheroid component, with little indication of a disk. There is a lack of features or distinct structures. Color gradients suggest some differential distribution of stellar populations. It is a red-sequence galaxy, with the bulk of its stellar population likely to be old. No prominent dust lanes or active star-forming regions are visible in the image. It is not currently undergoing any major mergers or interactions.
