The galaxy presents as a concentrated spheroid, appearing predominantly smooth with a high degree of central light concentration. Its overall shape is neither perfectly circular nor significantly elongated, exhibiting an intermediate ellipticity. There may be a slight distortion of its disk. The core exhibits a yellowish-white hue, possibly indicating an older stellar population, while the outer regions display a faint, greenish tint suggestive of the possibility of some ongoing, but relatively low levels of star formation. There is no obvious evidence of a major merger event. The galaxy exhibits a moderate redshift. This is a fairly large, bright galaxy.