The galaxy appears to be an elliptical type, exhibiting a smooth, concentrated light profile. The core is luminous and gradually fades into the outer regions of the galaxy, showing a soft, diffuse edge. The shape appears mostly rounded with a slight elongation and possible minor disturbances, implying a potential recent interaction with another galaxy. The color is primarily a yellow-orange hue, possibly indicating an older stellar population, with some bluer regions around the edges, suggesting ongoing, but relatively low, star formation activity within the disk. The galaxy is relatively compact, appearing approximately 8 kpc across.
