The galaxy presents a somewhat elongated morphology, suggesting it may be an elliptical galaxy or a spiral galaxy viewed at an angle. The central region exhibits a brighter, more concentrated light profile, likely indicating the presence of a galactic bulge. The outer regions show a gradual decrease in luminosity. There is evidence of a disk-like structure and possibly spiral arms. A faint blueish glow is visible in the disk and outskirts, possibly signifying regions of recent or ongoing star formation. Some disturbances seem to be present, possibly due to a minor merger or tidal interactions.
