The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal in shape. There is a concentrated central bulge that emits a bright yellowish glow, suggesting an older stellar population.  The outer regions of the galaxy show a gradual decline in luminosity. No distinct spiral arm structure or significant dust lanes are discernible. There is no apparent ongoing major merger or tidal disturbance visible, although slight asymmetries in the outer halo cannot be ruled out. The overall color profile suggests a passively evolving system with a low star formation rate.
