The galaxy presents as a spiral galaxy, likely a grand design type, observed at a redshift of approximately 0.139. It exhibits a notable central bulge, appearing moderately sized, with a smooth and concentrated light profile transitioning into a disk. Spiral arms are faintly visible, though not highly prominent, with an open morphology. The disk component appears to be the dominant feature. There is no obvious strong bar feature. Based on its morphology, the galaxy does not appear to be undergoing a major merging event, though subtle disturbances cannot be ruled out entirely. There is a slight asymmetry in the disk structure suggesting potential minor interaction. The galaxy has an estimated effective radius of approximately 6 kpc.
