The galaxy presents as a spiral type, exhibiting a disk structure with clearly defined spiral arms. The central bulge appears moderate in size and has a yellowish hue, suggesting a population of older stars. The spiral arms are prominent and winding with a tight distribution, displaying a bluish tint, indicative of ongoing star formation. Dust lanes are not particularly pronounced but subtle disturbances suggest possible minor interactions. Overall, the galaxy displays a well-defined structure, indicating it is not currently undergoing any major disruptive events.
