The galaxy exhibits a notable central bulge, appearing relatively smooth and concentrated. A fainter, extended disk-like structure surrounds the bulge. There is evidence of tidal distortion or interaction with another galaxy. This manifests as a disrupted morphology in the galaxy's outer regions, with hints of faint, extended arms or tails. The color suggests a mixture of stellar populations, with bluer regions potentially indicating ongoing star formation and redder areas suggesting older stellar populations. The galaxy seems to be involved in some sort of interaction that seems likely to lead to a major merger. Overall, the galaxy appears to be in a transitional stage, possibly evolving from a more regular spiral or disk galaxy into an irregular or elliptical system.
