The galaxy appears as a centrally concentrated, elongated object. It displays a smooth, elliptical morphology with a noticeable bulge in the center. The color distribution indicates an older stellar population, with a concentration of redder hues towards the central bulge. Fainter, bluer regions are observed toward the outer edges, suggesting some ongoing or recent star formation. The shape is consistent with an elliptical galaxy, although a slight disk component cannot be completely ruled out. No significant tidal features or signs of recent merger activity are immediately apparent in the image, but the possibility of minor disturbances is still a consideration.
