The galaxy presents as an elliptical morphology, with a smooth, concentrated light profile. Its overall shape approximates roundness, tending towards a slightly elongated form but exhibiting no prominent features indicative of a disk. The central region displays a significantly higher luminosity than the surrounding areas, suggesting a dense stellar population or active galactic nucleus. No major disturbances such as tidal tails or clear signs of an ongoing merger event are apparent. There is very little structure present. The colors of the galaxy appear to be skewed towards the red end of the spectrum, with a yellow to slight orange hue.
