The observed galaxy presents as a relatively large spiral galaxy, viewed at a high inclination. A prominent central bulge is clearly visible, exhibiting a yellowish hue, suggesting an older stellar population. Faint spiral arms extend from the bulge, appearing somewhat tightly wound. The disk component shows a bluer color, indicative of more recent star formation. A bar structure is present across the bulge of the galaxy. There are no obvious signs of a major ongoing merger, though minor disturbances cannot be ruled out. The galaxy has a relatively smooth appearance, but there is evidence for a more active formation of stars along the spiral arms.
