The galaxy presents as a spiral with a prominent bulge. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population. Surrounding the bulge is a disk component where faint spiral arms are present. The arms display a mottled appearance with blueish regions indicating areas of active star formation. Overall, the spiral arms exhibit a tightly wound morphology, suggesting a relatively old disk population as well. There appear to be at least two main spiral arms. The disk extends reasonably far from the bulge before fading into the background. There is no obvious sign of a strong bar feature. The galaxy appears relatively undisturbed.
