The galaxy presents as a spiral galaxy, observed at a redshift of z ≈ 0.02, indicating it is relatively nearby. There is a disk component with a central bulge, and the disk appears moderately inclined relative to our line of sight. The bulge has a prominent presence but does not dominate the overall morphology.

Spiral arms are discernible within the disk, exhibiting a somewhat flocculent structure rather than a grand design. The arms appear fairly open, and can be traced across a substantial portion of the disk. Star formation appears to be actively occurring in the spiral arms, as evidenced by the bluer colors associated with regions of ionized gas and young stars. There is no visual evidence suggesting a strong bar structure. There is no major merger or major disturbance, and it appears to be a relatively isolated system.
