The galaxy presents as a single, relatively smooth light source. It has an elliptical morphology, appearing mostly round with a slight deviation towards an intermediate shape. The galaxy exhibits a concentrated core, surrounded by a more diffuse halo. Color gradients are subtle, with the central region appearing bluer, indicating potential ongoing star formation, while the outer regions trend redder, suggestive of an older stellar population. There is no distinct disk structure visible. No major disturbances or signs of ongoing merger activity are apparent.
