This galaxy presents as a spiral structure with a noticeable disk component. The disk is not perfectly face-on but tilted somewhat relative to our line of sight. Prominent spiral arms are visible, exhibiting a patchy distribution of light, suggesting active regions of star formation. These arms appear tightly wound around the central bulge, with a somewhat flocculent structure.

The central bulge is moderately sized, appearing neither dominant nor negligible compared to the disk. A bar-like structure is suggested, with a hint of elongation across the central region.

There are indications of a possible interaction or minor disturbance occurring within the galaxy. It is not a violent merger, but there appears to be a slight asymmetry or warping of the disk shape.
