The galaxy presents as a centrally concentrated object with a relatively smooth appearance. The central region exhibits a yellow-white hue, suggesting an older stellar population. There is a lack of prominent spiral arm structures or distinct dust lanes, which indicates the likelihood of it being elliptical, or possibly a lenticular galaxy seen from a face-on angle. No significant tidal features or distortions are observed, suggesting the absence of recent major mergers or strong gravitational interactions. The galaxy appears moderately round. It may have undergone some prior disturbance, though the smooth appearance is dominant.
