The galaxy appears to be a relatively smooth, elliptical object with a high degree of roundness. Its light profile suggests a concentrated central bulge that gradually fades outwards. The color of the galaxy appears somewhat redder than galaxies that are actively forming stars. There are no obvious spiral arm structures or dust lanes visible. No signs of tidal disturbances or close companion galaxies are observed in the immediate vicinity, suggesting it is not currently undergoing a major merger event.
