The galaxy presents a generally smooth morphology, appearing largely elliptical in shape. The light distribution is concentrated towards the center, suggesting a prominent bulge. There is some subtle elongation observable in the image. A faint blueish tinge to the outer regions may indicate some ongoing, low-level star formation. There appears to be no significant dust lane or other clear indication of a disk structure. The overall structure suggests it is not currently undergoing any major merger activity, although there might be minor disturbances within the galaxy. The galaxy appears fairly round.
