The galaxy appears to be a spiral galaxy, presenting a near face-on orientation. The spiral arms are prominent, exhibiting a morphology consistent with a grand design spiral. The arms show a moderate winding, neither tightly wound nor extremely open. There are likely two primary spiral arms.

A bar structure is present within the central region, with an orientation spanning roughly vertically, and a strength that is difficult to discern from this image, but exists. The bulge is moderately sized, blending smoothly with the disk.

There is some visual evidence of interaction or disturbance in the outer regions of the galaxy, possibly indicating minor tidal effects. The colors within the disk suggest regions of active star formation, with bluer hues apparent along the spiral arms. There are no obvious signs of a major merger.
