The galaxy presents a generally elliptical morphology with a smooth light distribution. The central region displays a concentration of light, appearing yellowish or orange in color, suggesting an older stellar population. The outer regions exhibit a slightly bluer hue, indicative of younger stars and ongoing, but potentially low, star formation. The overall structure shows some degree of asymmetry, possibly a minor disturbance or interaction, however, there are no clear tidal tails or obvious signs of a major merger event. The galaxy's color profile suggests a transition from a redder core to bluer outer regions, which could mean inside-out quenching. Given the relatively smooth structure and slight blueness, it probably is an intermediate stage galaxy transitioning from being star-forming to quiescent.
