The galaxy presents an overall elliptical morphology. There is a smooth, centrally concentrated bulge, with a relatively uniform luminosity profile. No spiral arm structures are readily apparent. The color appears yellowish-white, suggesting an older stellar population dominating the galaxy's light emission. There is no discernible dust lane or regions of active star formation visible in this image. The galaxy exhibits a notable level of sphericity. No signs of ongoing or recent major merger events are evident. The galaxy appears undisturbed.
