The galaxy presents as a singular, relatively compact object. Its morphology appears largely smooth and elliptical, with a notable concentration of light toward the core. The overall color profile suggests a greater abundance of older stellar populations, likely with a reduced rate of ongoing star formation. There may be very faint signs of minor tidal disturbances, though these features are ambiguous. The galaxy exhibits a generally rounded shape, showing neither an obvious disk-like structure nor a highly elongated form.
