The galaxy presents as an elongated, disk-shaped structure, viewed nearly edge-on from our perspective.  A central bulge is subtly discernible, appearing as a region of concentrated light. The overall color appears to be bluish-white in the central regions, transitioning to a dimmer, more blue hue in the outer regions, suggesting active star formation. There appears to be some minor disturbances in its shape. The galaxy presents a smooth profile. The apparent symmetry of the disk indicates that it is a relatively undisturbed system with no major ongoing mergers, although minor interactions cannot be ruled out based on the image alone. 
