The galaxy appears to be a relatively smooth, elliptical galaxy. It presents a concentrated central bulge that transitions smoothly to a fainter outer halo or envelope. The color gradient suggests an older stellar population, potentially with ongoing but low levels of star formation. There is no distinct disk structure, spiral arms, or prominent dust lanes visible. The galaxy is generally round in appearance with no obvious signs of a major ongoing merger, though a minor disturbance cannot be completely ruled out.
