The galaxy presents as a flattened spheroid, with a clear major axis. The central region exhibits a concentrated, bright luminosity, indicating a high density of stars, likely an evolved stellar population, giving it a yellowish-orange hue. The luminosity smoothly decreases outwards from the center. The outer regions display a faint disk-like structure, but without clearly defined spiral arms. There is a slight blue tint to the very faint outer regions. The overall morphology suggests that the galaxy may be an elliptical, possibly transitioning from a spiral form. There is no apparent tidal disturbance, indicating it is not undergoing a major merger. It is a very compact galaxy. 