The observed galaxy presents a morphology consistent with a spiral galaxy, though the details are somewhat blurred. There is a discernible, moderately sized central bulge which appears yellowish, suggesting an older stellar population. Faint spiral arms emanate from this central bulge, though they are not sharply defined. The disk of the galaxy shows some patchy regions of bluer light, possibly indicating areas of ongoing or recent star formation. The galaxy is neither perfectly edge-on nor face-on, but rather at an intermediate angle of inclination. Overall, the galaxy's appearance is relatively undisturbed, suggesting no major recent merger events.
