The galaxy appears to be an elliptical galaxy, showing a smooth, centrally concentrated light distribution. There is little to no evidence of spiral arms or significant dust lanes. The galaxy exhibits a radial color gradient, appearing more yellow/orange towards the center and slightly bluer towards the outer edges. There is no visually apparent ongoing major merger activity, although subtle irregularities in the outer regions cannot be ruled out, potentially indicating minor interactions. Overall, the galaxy's morphology suggests an evolved system with a relatively old stellar population, with a low star-formation rate.
