The galaxy presents a somewhat amorphous, elliptical appearance. There is a bright central region that appears relatively smooth and concentrated. The outer regions exhibit a bluer hue, possibly indicating the presence of younger stellar populations or ongoing star formation within a disk-like structure. The overall morphology suggests a galaxy that may be in the process of transitioning from a more actively star-forming state to a quiescent state, though there is evidence of ongoing or recent star formation activity. The galaxy may be experiencing a minor disturbance or interaction, given its somewhat irregular shape and asymmetries in the outer regions. The galaxy does not appear to be strongly barred or have well-defined spiral arms.
