The galaxy presents a complex morphology indicative of a possible ongoing or recent merger event. The central region displays a moderate bulge, with an overall golden-yellow hue. The disk exhibits distinct spiral arm structures. A bar-like structure is visible across the central region.  The disk is not perfectly smooth; the presence of clumpy regions suggests regions of active star formation. The galaxy’s edge is not perfectly defined. There also appears to be tidal features surrounding the galaxy, indicative of a major disturbance event.
