The galaxy presents an elliptical morphology, with a smooth, diffuse light distribution that is concentrated toward the center. The core exhibits a bright, yellowish hue suggestive of an older stellar population. Extending outwards from the core is a more bluish halo indicating the presence of younger stars. The overall structure appears relatively undisturbed, showing no obvious signs of recent major merger activity, but there may be minor disturbances present. The galaxy is significantly elongated, deviating considerably from a circular shape, with the "in between" roundness being dominant. The estimated effective radius is around 5 kpc.
