The galaxy exhibits a generally elliptical morphology. The core region appears bright and relatively smooth. There are hints of a disk-like structure around the central bulge, though it is not well-defined. The light distribution suggests a degree of asymmetry or possible disturbance in the outer regions, with some indications of faint, extended features that could be tidal tails or debris from a minor merger event. Colors are notably bluer toward the edges of the galaxy. Some indication of internal structure with slightly mottled features is visible. The galaxy shows indications of low-level ongoing star formation.
