The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge. The light distribution appears to be dominated by older stellar populations, indicated by the yellowish-orange hue. No distinct spiral arm structures are discernible. The overall morphology suggests a system that has undergone significant dynamical relaxation. The galaxy appears moderately elongated, deviating from a perfect circular shape. There are no obvious signs of major tidal disturbances or ongoing mergers; however, subtle asymmetries cannot be ruled out at this resolution. The galaxy is a compact object, occupying a small angular extent. 
