The galaxy presents as a relatively smooth, compact structure with a dominant central bulge. It exhibits an ellipsoidal shape, appearing somewhat rounded rather than highly elongated. There's a slight hint of an extended disk or feature emanating from the main body, possibly indicating a faint spiral arm or tidal debris. The color distribution suggests a redder core, indicating an older stellar population. The outer regions appear bluer, potentially indicating recent star formation in these areas. There are no immediately apparent signs of ongoing major merger activity, although the slight asymmetry could suggest minor disturbances.
