The observed galaxy presents as a complex structure, potentially undergoing a merger event. The primary body of the galaxy exhibits a smooth, elliptical morphology, with a concentration of light towards the center. Three distinct, bright knots of luminosity are visible, suggesting either multiple galactic nuclei or intense regions of star formation. The tidal features, indicated by faint extensions and distortions, are indicative of gravitational interactions. These interactions suggest that the galaxy is currently merging. The color distribution shows a redder hue in the central region, possibly indicating an older stellar population or increased dust obscuration. The tidal extensions exhibit a bluer color, potentially highlighting younger stars formed during the interaction. The overall structure deviates from a regular disk or elliptical form, reinforcing the hypothesis of ongoing dynamical disturbance.
