The galaxy presents as a centrally concentrated object with a generally smooth morphology. The core region exhibits a bright, diffuse glow, indicating a high density of stars. There's a slight elongation or asymmetry in the overall shape. The galaxy appears to be in the process of a significant merger. There are noticeable tidal disturbances and asymmetrical features indicative of gravitational interaction. There's also evidence of multiple distinct nuclei or concentrations of stellar material, which would be consistent with an ongoing merger event. The redder color in certain regions may indicate older stellar populations or dust obscuration.
