The galaxy presents as a somewhat elongated, disk-shaped structure, likely a spiral galaxy observed at a significant inclination. Its central bulge appears prominent and exhibits a yellowish hue, indicating a population of older stars. The disk component displays a more diffuse, bluish color, suggesting the presence of younger, hotter stars and ongoing star formation. No distinct spiral arm structures are clearly visible. The overall appearance is relatively smooth, with only minor disturbances detected. The galaxy appears relatively isolated, showing no signs of a recent major merger event. The galaxy's color and morphology points toward intermediate levels of star formation. The galaxy is relatively large.
