The galaxy presents as a spiral type, observed at an oblique angle but not fully edge-on. Prominent spiral arms are discernible, exhibiting a morphology of two clear, winding structures. The spiral arms appear moderately open with a mixed distribution of tight and loose turns. There is evidence of active star formation within the arms, indicated by the bluish hue and patchy luminosity.

The central bulge is moderately sized in relation to the disk. The bulge appears yellow, suggesting an older stellar population. A bar structure is present. 

There appears to be no ongoing major merger, although subtle asymmetries in the arm structure hint at a potential minor interaction or disturbance in the past. The overall light distribution suggests that it has not undergone any recent major merger activity.
