The object appears to be a spiral galaxy, exhibiting a flattened disk-like structure. Faint spiral arms emanate from a central bulge. The arms show evidence of star formation, indicated by the presence of blue knots and a patchy, irregular texture. The central bulge has a moderate size relative to the overall disk. A bar may be present within the central region, though this is difficult to determine conclusively. The galaxy does not seem to have an edge-on orientation, but is more inclined. The winding of the spiral arms appear to be spaced loosely, and the arm count is hard to determine, but could be two, based on the symmetrical pattern. There do not appear to be major disturbances or indications of a merger event.
