The galaxy presents as a disk galaxy, observed at a significant angle of inclination. The central bulge appears relatively large and prominent, exhibiting a smooth, concentrated light profile. The surrounding disk is visible, though with a less defined structure. There are slight disturbances of the disk shape. A faint spiral arm structure can be faintly inferred within the disk. The color gradients suggest a moderate amount of recent or ongoing star formation, primarily within the disk. There is no strong evidence of a major merger.
