The galaxy presents an overall elliptical morphology. A bright, concentrated central bulge is observed, appearing nearly white in color. The inner disk is a bright cyan color, indicative of potentially strong [O III] emission and active star formation. Dust lanes are visible along the major axis on either side of the bulge, appearing a reddish hue. These dust lanes are relatively subtle and thin. The outer region of the galaxy appears bluer and more diffuse, suggesting a lower surface brightness and potentially a more extended stellar population. It exhibits a smooth structure with no apparent spiral arms or bar features. Indications are present that the shape may be due to an artifact. The galaxy is oriented edge-on with respect to our line of sight, obscuring a clear view of the galactic disk. Slight indications of disturbance may be present in the overall shape. 
