This galaxy appears to be a disk galaxy, viewed at a significant inclination to our line of sight. The central bulge is subtly visible, with a moderate degree of light concentration. A prominent, dusty disk is evident, obscuring the bulge region to some extent. There is a hint of spiral arm structure, exhibiting a flocculent, patchy morphology. The bluer coloration suggests active star formation regions, possibly concentrated within the arms. Evidence of minor disturbances are present, these may be satellite galaxies or tidal features.
