The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a concentrated, bright golden hue that transitions to a bluer, less intense halo. There's a slight asymmetry in the overall shape, with a hint of elongation along one axis, but it remains predominantly rounded. No distinct spiral arms or bar structures are discernible. Faint tidal features or indications of recent major merger events are not evident, although a minor disturbance cannot be ruled out. The smooth light distribution suggests a population of older stars dominates, indicative of a relatively quiescent star formation rate. The diameter is estimated to be around 4 kpc.
