The galaxy presents as a spiral, viewed at an angle between face-on and edge-on. The nucleus exhibits a bright, concentrated luminosity, suggesting a considerable stellar population and possibly an active galactic nucleus. A bar structure appears to be present, extending through the central region of the galaxy. The spiral arms are well-defined, showing a moderate winding, and appear somewhat flocculent in nature. The arms display a mottled texture with hints of blueish regions, indicating areas of active star formation. The overall color is dominated by older stellar populations in the bulge and inner disk. There appears to be a general symmetry in the spiral structure, without obvious major disturbances. The outer regions show a gradual decrease in luminosity.
