The galaxy presents as a somewhat elongated, elliptical structure. The central bulge exhibits a strong concentration of light, appearing a yellow-orange hue suggestive of an older stellar population. Fainter, bluer light extends outward from the core, possibly indicating regions of ongoing, low-level star formation. The overall morphology appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. There is a slight degree of asymmetry or faint arm-like features visible, though more data is needed to confirm their exact nature.
