The galaxy appears as an elongated, disk-shaped structure viewed nearly edge-on. A central bulge is subtly visible, appearing as a slightly brighter, more concentrated region. The disk itself exhibits a smooth texture, lacking prominent spiral arm features. The color gradient suggests a relatively older stellar population, with a general blue hue indicating some ongoing star formation. The object displays a slight inclination relative to our line of sight, offering a glimpse of its three-dimensional structure. Overall, the galaxy presents a well-defined and undisturbed morphology. There is no clear signs of recent mergers.