The galaxy presents a generally smooth, elliptical morphology. Its color profile indicates a dominant population of older stars, presenting a yellowish-orange hue in the central bulge. There is a subtle transition to slightly bluer tones in the outer regions of the galaxy, indicating the presence of some younger stellar populations, potentially associated with ongoing, but minimal, star formation. The galaxy appears relatively undisturbed with no obvious signs of recent major merger events or tidal features. It exhibits a well-defined central core, diminishing in intensity outwards. The overall light distribution is consistent with an evolved system undergoing a slow rate of star formation.
