The galaxy presents as a roughly elliptical structure with a bright, concentrated central bulge. The bulge appears yellow, possibly indicating an older stellar population. Fainter, bluer regions extend outwards from the bulge, suggesting ongoing star formation in a disk-like component. The disk appears relatively smooth, without prominent spiral arms or strong dust lanes. There are some indications of minor disturbances within the outer regions of the galaxy. The overall shape appears to be somewhat elongated, but generally rounded. There are no obvious signs of a major ongoing merger, though some subtle features may suggest a past interaction or minor disturbance.
