The galaxy presents as a spiral type with a central bulge. Spiral arms are visible, exhibiting a somewhat flocculent structure. There is a hint of a bar-like feature. The bulge appears moderately sized relative to the overall galactic disk. The disk exhibits blue hues, suggestive of ongoing star formation. The galaxy does not show any obvious signs of major interaction or merger events, but a few asymmetries are noticed. Overall, the galaxy appears to be an intermediate spiral type with moderate star formation activity.