This galaxy exhibits a generally smooth morphology. It appears to be largely spheroidal in shape, with a concentration of light towards its center. The color gradient suggests a higher concentration of older stars towards the galactic core, with bluer hues, indicating younger stellar populations, present in the surrounding region. There may be hints of a disk-like structure, though any defined spiral arms are absent. There are some slight irregularities in the outer regions, which may indicate minor past or ongoing interactions with another galaxy. Overall, the galaxy appears to be a relatively undisturbed system.
