The galaxy presents as a disk galaxy, observed at a slight inclination to our line of sight. There is a prominent central bulge, with a yellow/white color, indicative of an older stellar population. Surrounding the bulge, a disk is visible, displaying a bluish hue, potentially indicative of younger, hotter stars and ongoing star formation. There is a hint of spiral structure in the disk, although the arms appear somewhat ill-defined. The overall morphology suggests an intermediate type spiral galaxy. The galaxy appears relatively smooth, though with hints of some disturbances that could be the result of a minor merging event.
