The galaxy appears as a moderately bright, elliptical system. The central region exhibits a concentrated, luminous core that fades into a more diffuse halo. The galaxy appears largely smooth in texture, lacking any obvious spiral arm structures or distinct dust lanes. The overall shape is somewhat elongated. A faint reddish coloration is observed in some areas, suggesting the presence of older stellar populations. No significant tidal features or signs of ongoing major merger activity are readily apparent, although subtle disturbances cannot be entirely ruled out.
