The galaxy exhibits a clear spiral structure, characterized by well-defined arms emanating from a central bulge. These arms display a degree of winding, appearing moderately tight as they extend outwards. The presence of a bar-like structure is readily apparent within the central region, bisecting the bulge and influencing the organization of the spiral arms. The galaxy appears to be undergoing a significant interaction with another galaxy. There is a major disturbance to the morphology as a result of this interaction. The central bulge appears relatively prominent. Dust lanes are visible within the spiral arms. The galaxy displays a bluer hue in its outer regions, indicative of ongoing star formation. The structure shows considerable asymmetry, especially noticeable by the irregular shapes of the spiral arms and the disturbed bulge.
