This galaxy appears to be a spiral galaxy, presenting a somewhat inclined view relative to our line of sight. There is evidence of spiral arm structure, although it appears somewhat disrupted. A central bulge is not immediately discernible, potentially obscured by dust or the angle of observation.

The color distribution suggests active star formation regions throughout the galaxy, particularly in the spiral arms, indicated by the presence of blue and green hues. There is an apparent asymmetry in the overall structure, with one side of the galaxy appearing more disturbed or extended. This could be indicative of a past or ongoing interaction with another galaxy. 

There is a degree of patchiness, suggesting non-uniform distribution of stars, gas, and dust. The overall morphology suggests that the galaxy could be undergoing or recently experienced a merger event. 
