The object appears to be a spiral galaxy, exhibiting well-defined spiral arms. These arms are prominent and extend outwards from a central bulge, indicating a developed structure.

The galaxy is relatively face-on with only a slight tilt, allowing for a clear view of its overall morphology. There is evidence of ongoing star formation within the spiral arms, suggested by the presence of bright, blueish regions interspersed with areas of dust and gas.

The central bulge is not particularly dominant, suggesting that this galaxy is not an early-type spiral. The galaxy does not appear to have a strong bar-like structure, but subtle asymmetries exist in the morphology. 

There are disturbances evident in the outer regions of the galaxy. It may be interacting with a nearby galaxy. 

