The galaxy displays a moderately compact morphology, appearing somewhat amorphous in shape. The light distribution is relatively smooth, lacking a well-defined spiral structure. The central region exhibits a diffuse glow, with a slight suggestion of a central bulge. There may be some faint features indicative of a disk, but it is not sharply delineated. There are minor signs of disturbances within the galaxy. These could be caused by the interaction of the galaxy with another nearby object, or a minor internal restructuring. The overall color profile suggests a mix of stellar populations, with regions of bluer, presumably younger stars interspersed with redder, older populations.
