The galaxy presents as a smooth, elliptical-like morphology. It is elongated in shape, appearing significantly longer than it is wide. There is a concentrated central bulge exhibiting a bright, yellowish hue, suggesting an older stellar population. The color indicates low-level star formation within the galaxy. No distinct spiral arm structures or dust lanes are discernible within the image resolution. The overall appearance suggests a relatively undisturbed system, with no obvious signs of recent major mergers or tidal interactions.
