The galaxy appears as an elliptical system, exhibiting a relatively smooth and spheroidal morphology. The light profile shows a central concentration, gradually decreasing in intensity outward. The color gradient suggests an older stellar population, with a yellowish hue dominating the central region, possibly indicative of evolved stars. The absence of distinct spiral arm structures or significant dust lanes indicates a lack of ongoing major star formation. There is a slight asymmetry or possible disturbance in the outer halo region, which could be indicative of a minor merger event or tidal interaction, but is not significantly prominent to imply a full on merger. The galaxy overall presents as a quiescent system with a high degree of radial symmetry.
