The galaxy presents a generally smooth, elliptical morphology. It displays a concentrated central bulge that emits strongly in redder wavelengths, possibly indicating an older stellar population. The galaxy's overall color gradient suggests minimal recent star formation. The isophotes appear relatively undisturbed, with no obvious signs of major mergers or tidal features. A subtle, diffuse halo may extend beyond the main body, but it is not clearly defined within this image resolution. Based on its appearance, it is likely to be a massive galaxy, perhaps a lenticular or early-type spiral galaxy viewed at a significant distance. 
