The galaxy presents as an elliptical morphology with a relatively smooth light distribution. The core region exhibits a concentrated, bright, yellowish-white hue, suggesting an older stellar population. Moving outward from the center, the galaxy exhibits a gradual fading in luminosity, transitioning to a more diffuse, bluish halo. There is no evidence of spiral arm structure or significant dust lanes. Subtle asymmetries may be present, but the overall structure indicates a well-relaxed system. The overall impression is of an early-type galaxy at a moderate redshift.
