The galaxy appears to be an edge-on spiral, exhibiting a prominent disk-like structure. The bulge is quite noticeable, with a rounded morphology. There is evidence suggesting a significant merger event, possibly with another smaller galaxy or dwarf galaxy. This is manifested in the overall distorted shape of the disk and potential tidal features. These features suggest that there might be a high star formation rate.

The disk exhibits varying degrees of brightness along its plane, with the central regions appearing brighter and more concentrated. The galaxy's color profile indicates a mix of stellar populations, with bluer regions possibly associated with younger stars. Overall, the galaxy shows characteristics of an active system undergoing significant dynamical interactions and star formation.
