The galaxy presents a largely smooth and centrally concentrated morphology. Its shape appears generally elliptical, showing a slight deviation from perfect circularity. Color gradients are subtle, with a possible slightly bluer hue toward the outer regions. Evident features are largely absent, such as spiral arms or prominent dust lanes. The galaxy does not appear to be undergoing a major merger event based on visual inspection, although there is a hint of some minor disturbance. The overall light distribution suggests a relatively old stellar population, consistent with a low specific star formation rate.
