This galaxy presents an overall elliptical morphology, with a smooth, centrally concentrated light distribution. There is a noticeable color gradient, appearing more yellow/orange toward the galactic center and slightly bluer towards the outer regions. The galaxy does not display any prominent spiral arm structures or distinct dust lanes, lending credence to its classification as an elliptical galaxy. The isophotes suggest a slightly elongated shape, but not exceedingly so. There is no obvious sign of strong gravitational disturbance or ongoing major merger activity in this image. However, faint peripheral features cannot be completely ruled out without higher resolution imaging. The integrated light suggests an older stellar population with a relatively low current star formation rate, though there may be a small amount of more recent star formation occurring in the outer regions, based on the slight bluish tint observed there.
