The galaxy presents as a spiral type, exhibiting a distinct flattened disk structure. A prominent central bulge dominates the galaxy's core region, gradually fading into the surrounding disk. Two spiral arms emanate from the central region, tracing a curved path outwards. These arms appear relatively well-defined, suggesting a grand design spiral structure. The spiral arms exhibit a winding pattern of intermediate tightness. The galactic disk appears oriented close to face-on relative to the observer's line of sight. The galaxy does not appear to be significantly disturbed and the image does not provide a clear view of the bar.
