The galaxy presents as a spiral galaxy, exhibiting a disk-like morphology viewed at an oblique angle, indicating an inclination relative to our line of sight. A central bulge is discernible, appearing bright and yellowish. Spiral arms are present. Their winding appears mostly tight. The galaxy does not appear to be undergoing a major merger, nor does it display signs of significant disturbance, retaining a relatively undisturbed spiral structure. There is evidence of a slight asymmetry, which could be a faint tidal tail. The disk is noticeably flattened, with the semi-minor axis being considerably shorter than the semi-major axis. There is not any obvious bar structure present in the center of the galaxy.
