The galaxy presents as a fairly bright, elliptical object with a smooth, relatively featureless profile. Its core appears highly concentrated, exhibiting a distinct yellowish-white hue that suggests an older stellar population. The galaxy shows a well-defined, round shape with some hint of being slightly elongated, but not exhibiting a clear disk structure. There's no obvious sign of spiral arms or any recent major merging event. Faint color gradients suggest some variation in stellar population with radius, but the overall color remains consistent. The color suggests an older stellar population dominating with very low star formation rate. 
