The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated, luminous bulge that fades gradually into the outer regions. The overall color is a yellowish-red, indicative of an older stellar population with lower levels of ongoing star formation. No prominent spiral arms or dust lanes are discernible. There is a slight elongation in the galaxy's shape, but overall it appears close to round. There does not appear to be signs of any recent major merging events, though there may be very subtle disturbances present in the outer regions, potentially suggesting a minor interaction in the past.
