The galaxy appears to be composed of two distinct components, possibly indicating an ongoing or recent interaction. One component presents a smooth, elliptical structure with a concentrated central bulge. The color gradient suggests an older stellar population, concentrated towards the core. The second component, located above the first, exhibits a more irregular, disturbed morphology. It has a bluer hue, potentially indicating regions of active star formation. The overall structure suggests possible tidal distortions or ongoing merger activity, with evidence of disruption in the distribution of stellar material, which may indicate a gravitational interaction between the two components. The general appearance hints at a system undergoing dynamic evolution due to gravitational forces.
