The galaxy presents as a disturbed system, with a prominent central bulge exhibiting a reddish hue. A fainter, elongated structure extends from this central region, exhibiting a bluer color. Evident are signs of morphological disturbance in the form of irregular shapes and asymmetries. There is a noticeable lack of defined spiral arm structure. The galaxy exhibits a moderate level of star formation activity, as evidenced by the bluer regions, which are indicative of younger stellar populations. The general shape is neither completely smooth nor definitively disk-like, with the overall form appearing relatively elongated. There is strong indication of a possible ongoing or recent merger event. The presence of disturbed morphology suggests tidal interactions are at play.