The galaxy presents as a moderately luminous, disk-shaped structure with a generally smooth appearance. Its color profile reveals a central region that is yellow, suggesting an older stellar population. Moving outward from the core, the disk transitions to a bluer hue, indicative of ongoing star formation. The galaxy is observed at an angle, revealing its flattened shape, somewhere in between completely edge-on and face-on. There is no significant disturbance in the galaxy's morphology, although a slight asymmetry could indicate the potential presence of a companion galaxy or a past minor interaction. The galaxy does not exhibit any prominent spiral arm structure.
