The observed galaxy exhibits a morphology suggestive of interaction or a recent merger event. The central region presents a bright, relatively smooth component with a bluish hue, possibly indicating a population of younger, hotter stars. A distinct, somewhat irregular feature, rendered in magenta, is present near the core, which could suggest ongoing star formation within dust clouds. The galaxy appears slightly elongated, deviating from a perfect spherical shape. There is a component with more yellow light to the north. The overall structure indicates a system not fully relaxed into a stable, elliptical form, and might be in the process of dynamically evolving.
