The galaxy presents as a lenticular or possibly an elliptical galaxy, elongated in shape. It displays a smooth, concentrated central bulge that appears yellowish-orange, suggesting an older stellar population. The outer regions show a fainter, bluer hue, hinting at the presence of some younger stars or ongoing, albeit limited, star formation. There is no clear evidence of spiral arm structure. The morphology suggests a system undergoing passive evolution with only minor disturbances to its structure. Overall, the galaxy exhibits a relatively undisturbed form.
