The galaxy presents as a concentrated, luminous spheroid with a reddish-yellow hue dominating the central region. A faint, diffuse disk extends outwards from the core. The disk appears relatively smooth, lacking prominent spiral arm structures or distinct dust lanes. The galaxy exhibits a noticeable ellipticity, appearing somewhat flattened. No obvious signs of ongoing merger activity or major disturbances are apparent in this image, although some minor asymmetry is noticeable. The colour gradient suggests a population of older stars dominating the core region, which are consistent with minimal current star formation. 
