The galaxy presents an overall elliptical morphology, displaying a smooth, centralized luminosity profile. The color gradient suggests a concentration of older stellar populations toward the galactic center, shifting towards bluer hues in the outer regions. The system exhibits a slight cigar shape with no obvious presence of strong spiral arms. The disk-like morphology shows signs of modest star formation. There is no evident signs of tidal disturbances or recent major merger events. The galaxy appears relatively isolated, without immediate interacting companions.
