The galaxy presents as a spiral type, exhibiting well-defined spiral arms. These arms appear somewhat tightly wound towards the core and transition to a more medium wound pattern farther out. The nucleus displays a prominent bulge, but it doesn't dominate the overall structure of the galaxy. While there is not a strong bar, it's possible that a weak bar structure is present. The disk is oriented face-on relative to our line of sight. The arms display a blue tint implying active star formation. Overall, no signs of significant tidal disturbances or major ongoing mergers are evident; minor disturbances may be present. The galaxy showcases a mixture of old and young stellar populations and is actively forming new stars.
