The galaxy presents as a spiral galaxy, observed at a redshift of approximately 0.13. Its disk structure is clearly visible, exhibiting a moderate inclination relative to our line of sight, and a relatively high ellipticity suggesting a flattened morphology. The presence of spiral arms is strongly suspected, though definitive identification is difficult due to the limited image resolution, they appear somewhat flocculent. A distinct central bulge is observed, appearing to be moderate in size, contributing substantially to the overall luminosity of the galaxy. The bulge exhibits a smoother texture than the disk. The galaxy appears relatively isolated, showing no indications of ongoing major mergers.
