This galaxy presents a distinct spiral structure. The arms appear somewhat loosely wound and extend outwards from a prominent central bulge. This bulge exhibits a yellowish hue, potentially indicating an older stellar population.  The spiral arms display a more bluish coloration, suggestive of ongoing star formation. Two main arms are visually discernible, though fainter segments may indicate a more complex, multi-armed structure.  No strong bar feature is immediately apparent. The galaxy appears relatively undisturbed, without any obvious signs of major mergers or tidal interactions. The disk is not perfectly edge-on, allowing for the spiral structure to be observed. The overall morphology suggests a spiral galaxy with a moderate-sized bulge and active star formation within its spiral arms.
