The galaxy presents as an elliptical or lenticular system, appearing smooth and largely featureless. There is a central concentration of luminosity, suggestive of a prominent galactic nucleus. The galaxy exhibits a yellowish-orange hue, implying a population of older stars and a relative paucity of ongoing star formation. Its apparent shape is mostly circular, but the possibility of a slight elongation or mild tidal disturbance cannot be entirely ruled out. There is little evidence of spiral arms or significant dust lanes. The overall morphology suggests a relatively evolved system.