The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge, appearing approximately oblate in shape. There is a noticeable color gradient, transitioning from a yellowish-white core to a reddish-orange periphery. A subtle hint of a greenish hue is observed in regions surrounding the central bulge. There is no apparent spiral arm structure or dust lane features visible in this image. The overall light distribution suggests a population of older stars. There may be very minor disturbances visible. The galaxy shows a low rate of current star formation.
