The galaxy presents as a moderately luminous object with a generally elliptical morphology. A prominent central bulge is visible, appearing relatively smooth and concentrated, with a color gradient indicating potential variations in stellar population or dust content. The surrounding disk, while present, shows limited visible structure and arm definition. The disk appears to be tilted relative to our line of sight. There is a hint of some minor disturbance within the structure of the galaxy. Overall, the galaxy's smooth appearance suggests it is dominated by older stellar populations with low star formation activity.
