The galaxy appears as a relatively smooth and centrally concentrated elliptical type. It exhibits an overall elliptical shape, being somewhat elongated. The core region is intensely luminous, displaying a bright yellowish-white color, suggesting a population of older stars. Moving outward from the core, the light gradually fades into a more diffuse halo, with subtle color variations. These variations consist of faint bluish hues mixed with the dominant yellowish light, which could indicate some level of ongoing, but perhaps minimal, star formation. There does not appear to be evidence of strong spiral arm structures or distinct dust lanes. There are no obvious signs of any major ongoing merger events. The galaxy shows slight indications of disturbance.
