The galaxy presents a morphology indicative of a spiral galaxy, exhibiting discernible spiral arm structures. These arms appear somewhat loosely wound. A central bulge is visible, appearing to be of moderate size relative to the overall galactic disk. There is no evidence of a strong bar feature transecting the bulge.

The overall color profile suggests ongoing star formation, particularly within the spiral arms, indicated by the bluer hues. There is a smoother, yellower component contributing to the galaxy's overall light profile, likely associated with an older stellar population within the bulge. No significant tidal disturbances or indications of major merger events are readily apparent. 
