The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing mostly round, with a slight deviation. Color gradients are subtle but visible; the central region displays a yellowish hue, gradually transitioning towards a bluer color further out. There are no prominent spiral arms or distinct features, such as dust lanes, visible within the galaxy's structure. There is no noticeable tidal distortion or disruption, suggesting it is not currently undergoing a major merger event. The overall light profile indicates that the object is a substantial galaxy at a considerable distance, with ongoing, but not vigorous star formation.
