The galaxy presents as a moderately luminous, yellowish-orange elliptical system. It exhibits a relatively smooth morphology with no readily apparent spiral arm structure or significant dust lane obscuration. The galaxy's overall shape is somewhat elongated, appearing more 'in between' a perfect circle and a cigar-shape. There is no obvious indication of ongoing major merger activity, although subtle disturbances cannot be entirely ruled out. The galaxy is relatively compact. Based on its color, it appears to be comprised of older stars. The blue contribution is minimal.
