The galaxy presents a complex morphology. It appears to be an interacting system composed of at least two distinct components. The primary component is a relatively bright, flattened disk galaxy, oriented approximately edge-on. This primary disk exhibits a noticeable dust lane obscuring a portion of its central region, causing an apparent split. The light from this central region appears distinctly bluer than other parts of the galaxy. Fainter and more diffuse light appears extending from this central region in what may be tidal tails or galactic interactions.

A second component is visible adjacent to the primary disk, appearing as a more spheroidal, less structured entity. It is unclear if this component is actively merging with the primary disk, or if it represents a closely associated companion galaxy. This second component has a yellower color, potentially indicating an older stellar population. Overall, the system shows evidence of possible gravitational interactions, leading to morphological disturbances within the primary disk and potentially influencing the distribution of stellar populations.
