The galaxy presents as a centrally concentrated, smooth object. The core region exhibits a bright, yellowish-white luminosity, indicating a concentration of older stellar populations. The light smoothly diffuses outward with a redder tinge from this central core, with no apparent spiral arms or significant dust lanes. The overall morphology appears elliptical, exhibiting high degree of symmetry, consistent with a relatively evolved system. There is no evidence of active star formation. Small amounts of possible dust are observed within the surrounding galactic halo. There is no evidence of a recent major merger or significant tidal disturbance.
