The galaxy appears as a centrally concentrated, relatively smooth object with a round morphology. It exhibits a bright central region that gradually fades outwards. The color profile suggests a redder core transitioning to slightly bluer outer regions. There are no obvious signs of strong spiral arms or a well-defined disk structure; instead, the galaxy presents a generally amorphous form. There may be some indication of minor disturbance or interaction, given the somewhat uneven distribution of light in the outskirts, but it lacks any clear signs of a major merger event. Overall, the galaxy seems to be an elliptical-type galaxy or a smooth disk galaxy. Star formation rate appears low, the mass of the galaxy is very high.
