The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge and a surrounding halo. The core of the galaxy exhibits a bright, yellowish-white glow, suggesting a high density of older stellar populations. The surrounding halo is less intense in color and brightness, fading into the background with no obvious distinct edges. There are no visible spiral arms or dust lanes, which supports its classification as an elliptical galaxy. The overall shape appears to be round. There is no evidence of any ongoing merging events or major tidal disturbances.
