The galaxy appears to be undergoing a significant interaction, potentially a merger event. Two distinct structures are visible. The larger, primary component displays a smoother morphology with an elliptical shape. Its color gradient indicates an older stellar population, with a core that exhibits a redder hue. The smaller secondary component exhibits a bluer color, suggesting the presence of younger stars and ongoing star formation. There is evidence of tidal distortion, with faint extensions and asymmetric features hinting at gravitational disruption due to the interaction. The overall luminosity suggests a galaxy of considerable mass, with a moderate rate of star formation.