The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution. The shape is generally round, showing minimal deviation from circular symmetry, and no obvious disk structure. There is no sign of tidal tails, dust lanes, or other features suggesting a recent or ongoing merger event. The color profile appears somewhat uniform, with a slight reddening towards the center of the galaxy. Based on its apparent magnitude, the galaxy is intrinsically luminous. Star formation rate estimates are present, indicating moderate levels of current star formation activity. The object's size is small, possibly indicating that it is a compact elliptical galaxy.
