The galaxy exhibits a disk-like morphology, although the disk appears to be disturbed or irregular. There's a noticeable central bulge, which contributes to the galaxy's overall luminosity. The galaxy appears to be relatively blue in color, which may indicate ongoing star formation. The outer regions of the galaxy are less defined, suggesting a gradual decrease in stellar density. There's some evidence of possible merging or tidal disruption in the galaxy's structure. This may have led to the irregular shape and disturbed disk.
