The galaxy presents as a somewhat elongated, disk-shaped structure viewed at a moderate inclination. A central bulge is evident, appearing as a bright, concentrated region of light. The disk exhibits spiral arm features, which appear somewhat tightly wound. There is a faint bar-like structure that spans a considerable amount of the galaxy. The outer regions of the disk appear less defined, with a gradual decrease in surface brightness extending into the surrounding space. The galaxy displays a smooth light distribution, suggesting it is dominated by older stellar populations, although some areas are more blue in color, showing hints of star formation within the spiral arms. The galaxy exhibits no signs of strong tidal disturbances. The object appears to be isolated.
