The galaxy presents a morphology indicative of a spiral type. The central bulge appears moderately prominent, surrounded by a disk structure. Distinct spiral arms are visible, displaying a predominantly two-armed structure. The arms exhibit a loose winding pattern. There is some evidence of a bar-like structure extending through the central region. The galaxy shows a blue hue, especially in the spiral arms, possibly indicating active star formation. The disk appears relatively undisturbed, with no obvious signs of major mergers or tidal disruptions.
