The galaxy presents as a somewhat elongated, elliptical morphology. Its light profile appears relatively smooth, lacking significant defined spiral arms or a prominent central bar. The core exhibits a yellowish-orange hue, suggesting an older stellar population dominating this region. Progressing outward from the core, the galaxy appears to fade into a fainter, diffuse halo. Overall, there is no obvious evidence of major recent merger activity, though the galaxy does not appear perfectly circular and does exhibit some irregularities, hinting at potentially minor gravitational interactions or disturbances.
