The galaxy presents as an elliptical morphology with a high degree of central concentration. The galaxy's light profile appears smooth, lacking prominent spiral arms or distinct features. The galaxy exhibits a slightly elongated shape, although it appears mostly round. There is a slight color gradient observed, with the core exhibiting a more yellowish or gold hue, suggesting an older stellar population. Fainter, blueish emissions appear on the outskirts of the galaxy, possibly indicating recent, localized star formation. The galaxy shows no visible signs of ongoing merger activity or major disturbances, such as tidal tails or strong asymmetries.
