This galaxy exhibits a relatively smooth morphology, appearing largely featureless. The light distribution suggests a centrally concentrated spheroid, with a generally round shape. There is a slight asymmetry in the galaxy's overall form, suggesting a possible minor gravitational disturbance. The galaxy displays a color gradient, with the central region appearing more yellow, transitioning to a redder hue in the outer regions. This color gradient suggests a possible radial variation in stellar populations or dust content. The lack of prominent spiral arms or a distinct disk structure supports a classification as an elliptical galaxy. The apparent smoothness and color profile indicate that star formation may be currently suppressed.
