The galaxy appears to be a spiral galaxy, viewed at an angle. The central bulge is prominent and exhibits a yellowish-white color, suggesting an older stellar population. Fainter, bluish-white spiral arms extend from the bulge, indicating the presence of younger stars and ongoing star formation. The disk exhibits a moderate degree of ellipticity and shows a slight warping. Overall, the galaxy possesses a relatively smooth, well-defined structure, showing no immediate signs of major disturbances or mergers, though a potential minor interaction can't be ruled out. The galaxy is of intermediate redshift, indicating that the light we observe has been stretched to longer wavelengths as it traveled through the expanding universe.