The galaxy presents as an elliptical morphology, with a smooth and centrally concentrated light distribution. The light appears more concentrated toward the center. The color suggests an older stellar population, exhibiting a redder hue in its core that fades into a slightly bluer halo. There is a lack of prominent dust lanes or spiral arm structures. The object's elongation is not substantial, suggesting it is closer to round than a highly elongated elliptical. There are no visible signs of major interactions or mergers affecting its overall structure, though there is very minor disturbance. The galaxy appears to be relatively isolated in the image.
