The galaxy presents as a centrally concentrated object with an elliptical morphology. Its light profile appears smooth, with no obvious spiral arm structures or dust lanes visible at this resolution. The core of the galaxy exhibits a yellowish-orange hue, suggesting an older stellar population and a relative lack of ongoing star formation. The outer regions show a gradual fading in intensity and a subtle shift towards redder colors, further indicating an aging stellar population. The galaxy's overall structure appears undisturbed, with no signs of recent major merger events or tidal distortions. Faint extensions around the galaxy are likely present, but difficult to detect due to the image quality. The galaxy's size is estimated to be roughly 14 kiloparsecs in diameter.
