The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated luminosity profile. The core region appears brighter and more intensely colored with a slight reddish-yellow hue, potentially indicating a population of older stars. The galaxy shows a gradual decrease in light intensity moving outward from the center. The surrounding halo is bluish in color, suggesting the presence of a younger stellar population contributing to the overall light. The galaxy appears relatively undisturbed, lacking prominent tidal features or signs of recent major merger events. There is a hint of a very slight asymmetry in the outer halo, possibly suggestive of a minor interaction or accretion event in the past.
