The galaxy presents as a somewhat elongated, spindle-shaped structure. Its morphology appears to be relatively smooth, with minimal signs of significant disturbances. The color gradient suggests some variation in stellar populations or dust content across the galaxy's extent. A slight blueish tinge is visible in the central regions, possibly indicating ongoing star formation. The overall form is consistent with a disk galaxy viewed at a high inclination, approaching edge-on. The general appearance points towards a mature system that has largely settled into a stable configuration.
