The galaxy presents as a relatively smooth, elliptical morphology. Its light is concentrated towards the center with a distinct bright nucleus. The color profile suggests an older stellar population; the light emitted is in the yellow-redder part of the spectrum, indicating fewer young, hot stars. The galaxy's overall structure lacks prominent features like spiral arms or significant dust lanes. It appears fairly undisturbed, exhibiting no signs of major ongoing mergers or tidal disruptions. The galaxy seems to be of considerable mass. There is low star formation.
