The galaxy presents as an elliptical or lenticular structure, exhibiting a high degree of central concentration. A smooth luminosity profile is observed, with a relatively featureless disk. The dominant color is a yellowish-orange hue. There may be minor distortions of its structure indicative of past gravitational interactions. The galaxy appears relatively round. There are no strong signs of active star formation based on the image data. There may be some minor disturbance in the morphology, indicating it may be undergoing or have undergone a minor merger.
