The galaxy presents a morphology suggestive of a disk galaxy, although the bulge component appears significant and centrally concentrated. The overall color is yellowish-white, potentially indicating an older stellar population. The disk appears somewhat disturbed or irregular. There's a hint of possible tidal features or minor distortions, and a slight asymmetry in the distribution of light within the disk. A small amount of ongoing star formation is likely taking place. There is no indication of any recent or major merger activity, but a minor disturbance cannot be ruled out. 
