The galaxy presents as a spiral type, exhibiting a discernible disk structure. The spiral arms appear prominent, loosely wound around a central bulge. The bulge appears moderately sized relative to the disk. There is no evidence of a strong bar structure, and the presence of a weak bar cannot be conclusively determined from the image. The color gradient suggests active star formation within the spiral arms, indicated by a bluer hue, while the central bulge exhibits a yellower, older stellar population. There is no obvious sign of a major ongoing merger or significant tidal disturbance. Overall, the morphology suggests a relatively undisturbed spiral galaxy with ongoing star formation.