The galaxy presents a relatively compact structure. It appears predominantly smooth in texture, with a noticeable concentration of light toward the central region. The overall shape is neither perfectly spherical nor highly elongated, exhibiting an intermediate form. There is no strong evidence of spiral arm structures or a distinct disk component visible within the galaxy's morphology. Minimal distortion suggests a lack of major ongoing merger events. The light distribution transitions smoothly from the core to the outer regions. A slight asymmetrical feature is observed in the distribution of light.