The galaxy presents as a spiral type with a moderate inclination relative to our line of sight. A central bulge is evident, exhibiting a yellowish-white hue, suggesting a relatively older stellar population. The spiral arms are well-defined but somewhat flocculent in nature, displaying a bluish tinge, indicative of ongoing star formation. There is no indication of a strong central bar structure. The arm winding appears moderate. There does not seem to be any presence of major merging or tidal disturbance. The morphology suggests a late-type spiral galaxy with ongoing star formation activity.
