The galaxy exhibits a generally smooth morphology, though there are some features suggestive of a disk. The object's light profile displays an elliptical shape, with a brighter central bulge region that is characterized by a yellowish-red hue. Fainter extensions appear to be present, possibly suggestive of spiral arms, though they are not well-defined. There seems to be a very low rate of current star formation. The overall structure seems to be relatively undisturbed, with no obvious signs of a major merger event. A minor gravitational disturbance is possible. The light distribution from this galaxy suggests it is a massive object. 
