The galaxy appears to be a relatively smooth, elliptical shape, exhibiting a central bulge that is brighter and more concentrated. The light from the bulge has a yellowish tint, potentially indicating an older stellar population residing in that region. Extending outward from the core is a fainter, bluer halo, possibly indicative of more recent or ongoing star formation. There are some very faint hints of asymmetries or irregularities in the outer regions, though they are subtle. The overall structure suggests a galaxy that is relatively settled and not undergoing major mergers, but might have undergone a minor interaction in the past, given the disturbance fraction.
