This galaxy appears to be a spiral galaxy, possibly undergoing a merger or significant interaction with another galaxy. The structure is characterized by two distinct luminous regions, each exhibiting a spiral arm morphology. One of these regions is more compact and brighter, likely representing the primary nucleus or a region of intense star formation. The other is more diffuse, and the spiral arms appear less defined. The color gradient within the galaxy suggests a range of stellar populations, with the brighter, central regions exhibiting yellowish hues.

The arms themselves are not tightly wound. There is a moderate bulge component present. The overall shape appears elliptical with a degree of asymmetry. The galactic disk is inclined relative to our line of sight.
