The galaxy appears as an elongated, lenticular or early-type spiral galaxy. It exhibits a relatively smooth, centralized light distribution, with a bright nucleus. The color gradient suggests an older stellar population, primarily composed of evolved stars. There is a subtle hint of disk-like structure, though it's not strongly defined and appears more like a gradual flattening than a distinct, separate component. No significant dust lanes or prominent star-forming regions are visible in this image.
