The galaxy appears to be a lenticular or elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution. The object possesses an elongated shape, suggesting a flattened spheroid. The core region displays a yellowish hue, potentially indicating an older stellar population. Surrounding this, a bluer color can be observed, suggesting possible areas of some younger stars. No clear spiral arm structures or distinct dust lanes are visible within the observable features of this galaxy. Based on the galaxy's undisturbed morphology, there is a low probability of recent major merger activity.
