The galaxy appears to be an elliptical galaxy, showing a smooth, featureless profile with a centrally concentrated bulge. There is a slight elongation. The color distribution suggests an older stellar population. The lack of distinct features, such as spiral arms or dust lanes, supports the classification as an elliptical galaxy. The galaxy is relatively round. There is only a minor disturbance to its structure. The galaxy has an estimated size of 4 kiloparsecs. The magnitude measures suggest the galaxy is brightest in the z-band, followed by the r-band, and dimmest in the g-band. The galaxy is emitting at a low rate of star formation. The stellar mass is high.
