The observed galaxy presents as a disk-shaped structure, viewed at an oblique angle, not quite edge-on. There is evidence of spiral arm structure, though the arms are not sharply defined, suggesting a flocculent or patchy morphology. The central region exhibits a bright bulge component which appears to be moderate in size. The color profile suggests a degree of ongoing star formation, particularly within the disk where a blue hue is noticeable. The galaxy does not show strong evidence of a bar structure. There is no readily apparent major merger event occurring, though some minor tidal disturbances may be present within the galactic disk. The overall impression is of a spiral galaxy with a mix of established stellar populations and recent star formation.
