The galaxy presents a discernible disk-like structure, though the arms are not sharply defined. It exhibits a central bulge that appears relatively large and luminous, with a color profile that suggests an older stellar population. The disk surrounding the bulge shows some subtle color variations, possibly indicating regions of ongoing or recent star formation. The overall morphology suggests an intermediate stage between a spiral and a lenticular galaxy. There is some subtle warping and faint light outside of the main disk which could indicate minor gravitational disturbances. The galaxy appears to be relatively massive and undergoing a moderate amount of star formation.
