The galaxy exhibits a morphology consistent with that of a spiral galaxy viewed at a slight angle to face-on. A central bulge is visible, appearing moderately bright and concentrated. Faint spiral arms emanate from the bulge region, appearing tightly wound. The disk component appears bluish, suggestive of ongoing star formation. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major mergers or significant tidal interactions. The galaxy exhibits moderate central concentration. The spiral arms are somewhat difficult to resolve in detail, suggesting a relatively smooth stellar distribution within the disk.
