The galaxy presents as a diffuse, moderately elongated object with an apparent disk-like structure. There is evidence of a slightly disturbed morphology, possibly indicating an interaction or merger event. The central region appears somewhat smoother, transitioning into fainter and more irregular outer regions. The color distribution suggests active star formation regions, particularly along the disk, interspersed with older stellar populations. There's a hint of tidal features or disrupted arms extending from the main body. The overall luminosity is low.
