The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. A bright, yellowish core is evident, suggesting an older stellar population dominates the central region. Fainter, bluer extensions surround the core, possibly indicating some level of recent star formation in the outer regions. The galaxy exhibits a notable degree of ellipticity, appearing somewhat flattened. There is no obvious presence of spiral arms or a prominent disk structure. Overall, the galaxy appears relatively undisturbed, without clear signs of ongoing major mergers or tidal interactions.
