The galaxy presents as a grand design spiral, observed face-on. Two prominent spiral arms emanate from a bright, yellowish central bulge. The arms are well-defined and exhibit a moderately wound structure, appearing relatively symmetrical. The spiral arms show a mottled texture, suggesting active star formation regions and dust lanes. The central bulge appears significant in size relative to the disk and is generally smooth in appearance. The galaxy does not show any obvious signs of a major merger, although some minor disturbances or tidal features cannot be ruled out based on this image alone. A bar structure may be present, but if so, it is subtle. The overall color profile suggests a mixed stellar population, with a concentration of older, redder stars in the bulge and bluer, younger stars in the spiral arms. The disk component dominates the galaxy's overall appearance.
