The galaxy presents as an elongated, disk-shaped structure viewed nearly edge-on. A central bulge is apparent, exhibiting a concentration of light that suggests a high stellar density. This bulge appears to be ellipsoidal in shape. The galactic disk extends outwards from the bulge, appearing relatively smooth and lacking prominent spiral arm features. The disk material is likely composed of dust, gas, and stars. There is evidence of a blueish hue distributed across the body of the galaxy, particularly in the outer regions of the disk, which may indicate ongoing star formation. The overall morphology of the galaxy suggests a relatively quiescent state, with a smooth structure and minimal evidence of recent major mergers or interactions.
