The galaxy exhibits a relatively smooth morphology with a centrally concentrated light distribution. The galaxy is roughly elliptical in shape, appearing slightly elongated. The color profile indicates a population of stars that are actively forming, evidenced by the blue hue surrounding the central region. The galaxy's structure suggests there is likely a supermassive black hole residing at its center. There are signs of minor disturbances, which suggests a previous or ongoing interaction with a smaller companion galaxy. The presence of such disturbances indicates that the galaxy may be undergoing a merger.
