The galaxy presents as a spiral type, exhibiting distinct spiral arm structures. The arms are well-defined, tracing a relatively tight winding pattern around a central bulge. The bulge appears moderately prominent. A bar structure is subtly observed, which suggests the presence of a barred spiral galaxy. The galactic disk is oriented face-on, allowing a clear view of its spiral morphology. No obvious signs of major merging events or significant tidal disturbances are apparent. The disk exhibits a blueish hue, especially in the spiral arms, indicating ongoing star formation activity. Overall, the galaxy appears to be a well-formed spiral with a significant bulge and actively forming stars.