The galaxy presents as a concentrated, yellowish-orange object. Its structure appears largely smooth and elliptical, with indications of ongoing or recent merging activity, possibly with a companion galaxy. The main body exhibits a relatively high degree of circularity, with a slight elongation. There is evidence of disturbances in the overall form of the object, suggesting a possible gravitational interaction. The color suggests an older stellar population dominates, indicating a relatively low current star formation rate. The galaxy is a significant distance away from our own.
