The galaxy appears to be a relatively smooth, elliptical type. It presents a concentrated central bulge that is yellow-white in color, indicating an older stellar population. The surrounding halo or disk appears less prominent and displays a faint blue hue, possibly indicating some ongoing star formation. The overall shape is somewhat elongated but not strongly so, leaning towards spheroidal. There is no obvious evidence of spiral arms or significant dust lanes, nor any significant tidal disturbance to suggest a recent major merger. However, some faint irregularities could potentially suggest minor interactions. The galaxy is relatively compact.
