The observed galaxy presents as a spiral type, displaying a defined disk structure. The presence of spiral arms is evident, though their exact count is ambiguous due to limited resolution. The arms exhibit a moderate winding pattern, suggestive of differential rotation within the disk. A pronounced central bulge dominates the galaxy's core, displaying a yellow-white hue that implies an older stellar population. A strong bar feature transects the bulge region, appearing to disrupt the symmetric profile of the bulge. There is a ring surrounding the bar and bulge structure. The disk shows some hints of ongoing star formation, but this is largely concentrated to the outer portions of the arms. The disk inclination presents a near face-on orientation. There are some potential signs of minor tidal disturbances, though conclusive evidence for a major merger is not apparent.
