This galaxy appears as a somewhat elliptical, moderately concentrated luminous object. The light distribution seems relatively smooth across the body of the galaxy, with no immediately obvious spiral arm structures or dust lanes visible in the image. There is a slight elongation, and the galaxy does not appear perfectly circular. The overall color is consistent with an older stellar population. The central region is slightly more luminous compared to the outer parts of the galaxy, which suggests a central concentration of stars. The galaxy seems undisturbed without any visible tidal features or signs of recent major merger events. However, it may have undergone a minor merger event at some point in its past. This galaxy is a relatively massive system, displaying a subdued star formation rate. 
