The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a high degree of central concentration, with a gradual decrease in surface brightness outward from the core. The galaxy appears to have a near-spherical shape, with only a slight deviation towards an elongated form. There is no readily apparent spiral structure or distinct disk component. The color profile suggests an older stellar population, particularly in the central regions, with a possible presence of dust. No major disturbances or tidal features are visible, suggesting a relatively isolated and quiescent system. There is an extremely slight indication of a potential minor interaction or disturbance.
