The galaxy presents a largely smooth morphology, appearing relatively featureless at this resolution. It is centrally concentrated with a diffuse, extended halo. The light distribution suggests a spheroid-dominated structure, possibly an elliptical galaxy or a lenticular galaxy seen face-on. There is a slight elongation in its shape. The color profile appears redder, indicative of an older stellar population. A small area of possible star formation is visible as a bluer region. The galaxy doesn't show signs of major disturbances or ongoing mergers, though there are small, subtle irregularities.
