The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light profile gradually diminishes from the bright core outwards, suggesting a centrally concentrated distribution of stars. There's minimal evidence of spiral arm structures or significant dust lanes. The overall color appears yellowish-white, indicating a stellar population dominated by older, cooler stars. No signs of strong star formation regions are apparent within the visible spectrum of this image. There are no prominent tidal tails or other morphological disturbances, which suggests it is not currently undergoing a major merger, or is in the late stages of one.
