The galaxy presents a generally smooth, elliptical morphology, appearing somewhat rounded in shape. There is a concentrated central bulge that appears to be largely composed of older stellar populations, as indicated by its yellow-red hue. The outer regions fade smoothly into the background, showing no prominent spiral arms or disk features. Minor irregularities may be present in the outer envelope, possibly suggestive of tidal interactions or minor disturbances. The color profile suggests a lack of significant ongoing star formation.
