The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is little evidence of distinct spiral arms or significant dust lanes. The light distribution is centrally concentrated. The galaxy exhibits a color gradient, with the central region appearing more yellowish-orange and the outer regions exhibiting bluer hues. There is some potential presence of minor morphological disturbances, but they are subtle and could also be artifacts of the imaging process. Overall, the galaxy appears to be an evolved system with a relatively quiescent star formation rate, implying a potential transition towards a red-and-dead state.
