The galaxy presents as a somewhat smooth and elliptical object. Its light profile appears centrally concentrated, with a bright core that fades gradually outwards. Color gradients suggest an aging stellar population concentrated in the bulge.

There is faint evidence of a possible disk structure, although its morphology is not well defined and may just be a weak spiral. This galaxy is elongated and appears to have an intermediate roundness. No major mergers or disturbances are apparent in this image.
