The galaxy presents as a spiral type, viewed at a considerable inclination angle, but not quite edge-on. There is some evidence of tightly wound spiral arms visible within the disk. The central bulge is moderately sized and has a dominant golden hue, suggesting an older stellar population. The disk exhibits a bluer color, indicating regions of ongoing star formation. There is no obvious evidence of a strong bar structure bisecting the galactic center. Furthermore, there are no obvious signs of major mergers or significant tidal disturbances affecting the galaxy's morphology.
