The galaxy presents as a single, centrally concentrated object with a smooth, largely featureless morphology. Its overall shape is elliptical or spheroidal, appearing nearly circular. The central region exhibits a high surface brightness, gradually decreasing outward. Color gradients are subtle, with the core appearing slightly more yellow, transitioning to a redder hue in the outer regions, suggesting an older stellar population. There is no obvious evidence of spiral arm structure, a bar, or significant dust lanes. Additionally, there are no obvious signs of tidal tails or distortions indicative of a recent major merger event.
