This galaxy presents as a barred spiral with a moderate bulge component. The spiral arms are loosely wound and somewhat flocculent, displaying a predominantly two-armed structure. The bar feature is prominent, extending through the galactic center. The galactic disk is viewed at an angle, not quite edge-on. There appears to be some star formation occurring within the spiral arms, as evidenced by regions of bluer light. Overall, the galaxy exhibits a disk-dominated morphology with a relatively smooth appearance beyond the spiral arm structures. There's no obvious evidence of significant tidal disturbances or ongoing major merging events. The galaxy is relatively faint and distant.