The galaxy appears to be a relatively smooth, disk-shaped system. The central region exhibits a bright, concentrated core, suggesting the presence of a significant stellar population or an active galactic nucleus. The disk component shows a gradual decrease in surface brightness away from the center. There may be some subtle irregularities or disturbances in the outer regions of the disk, but these are not pronounced. The color gradient indicates some level of active star formation. The overall morphology is more elliptical than circular, showing a cigar shape. There are no obvious signs of a recent major merger or strong tidal interactions.
