The galaxy exhibits a morphology consistent with a spiral type, showing distinct, though somewhat tightly wound, spiral arms. The central bulge appears moderate in size, displaying a yellowish hue suggestive of an older stellar population. The spiral arms are less organized, some light disturbances can be seen throughout the spiral arms. A bar-like structure cannot be determined. The overall form is clearly disk-dominated, with a slight tilt relative to our line of sight. The disk regions appear bluer, indicating the presence of ongoing star formation.
