The galaxy appears to be a disk-shaped system, seen at an oblique angle. It exhibits a bright, concentrated central bulge region which fades out into the disk. The inner bulge is slightly elongated, with a smooth appearance and a warmer hue, suggesting an older stellar population. Fainter arms are suggested within the disk, displaying a blue-green color suggesting active star formation. The disk appears relatively smooth and well-defined, suggesting the absence of any major recent mergers or tidal disruptions. The morphology is consistent with an intermediate-type spiral galaxy transitioning from a disk system with a prominent bulge to a spiral disk system. 
