The galaxy appears to be a relatively smooth and centrally concentrated object. The light distribution suggests a spheroidal morphology, possibly an elliptical galaxy or a lenticular galaxy viewed at a moderate inclination. The core exhibits a bright, slightly yellowish hue, transitioning to a fainter, bluer color in the outer regions. There is no obvious spiral structure or distinct dust lanes visible. The overall form suggests a system dominated by older stellar populations with ongoing, albeit relatively low, star formation activity. There is a subtle hint of asymmetry or minor disturbance on the periphery, possibly indicating a past or ongoing minor interaction or merger event. The light is fairly concentrated.
