The galaxy presents as a slightly elongated, elliptical-like structure. Its core exhibits a high degree of central concentration, appearing smooth and predominantly yellow. The outer regions show a more diffuse and less structured distribution of light, also trending towards yellow and redder hues. There is a possible minor disturbance or merging event visible as a slightly brighter and more compact region on one side of the galaxy. The overall morphology suggests a lack of significant ongoing star formation. The galaxy appears to have a substantial mass, judging by its overall luminosity.
