The galaxy exhibits a spiral structure, with prominent arms extending outwards from a central bulge. The spiral arms appear tightly wound in some regions and more open in others. Star formation is evident along the arms, indicated by the presence of bluer regions likely containing young, hot stars. A bar-like feature is visible crossing the central bulge, and there appears to be evidence of tidal disturbances, suggesting a potential interaction or merger event. The dust lanes are relatively distinct, with some obscuring portions of the bulge and arms. The disk is tilted considerably, with some of the arms obscured and others quite visible. The interaction makes it hard to assess what is happening in the disk of this galaxy. The main bulge of the disk is also clearly visible, and appears to be yellow, as expected.
