The galaxy appears as a centrally concentrated object with a smooth, rounded morphology. There is no clear evidence of spiral arm structure or a pronounced disk component. The light profile suggests a relatively uniform distribution, typical of an elliptical or lenticular galaxy. The galaxy exhibits a faint, diffuse halo extending outwards from the bright central region. There may be some very minor disturbances present, but the overall structure does not suggest a major recent merger event. The color is slightly more blueish in the center, which suggests on-going, but minimal, star formation.
