The galaxy presents a smooth, elliptical morphology. The central region exhibits a bright, concentrated core, indicating a substantial stellar density and possibly the presence of a supermassive black hole. The light profile appears to fade gradually from the center outward, lacking distinct spiral arm structures. The overall color of the galaxy is somewhat red, suggesting an older stellar population with a lower rate of ongoing star formation. There is no evidence of significant dust lanes or tidal features, indicating it is a relatively undisturbed system, and showing little evidence of a recent major merger. The galaxy appears well-defined and undisturbed, with no nearby companions influencing its shape.
