The galaxy appears to be a relatively smooth, elliptical galaxy. The light is centrally concentrated with a high degree of radial symmetry, exhibiting a gradual decrease in intensity from the core outwards. There is no strong evidence of spiral arms or a prominent disk structure. The galaxy displays a slightly bluish hue near its core, subtly shifting towards redder tones in its outer regions. There is no immediately visible dust obscuration or signs of significant tidal disturbances.
