The galaxy presents a primarily smooth morphology, with a general elliptical shape and a high degree of central concentration. Its color profile suggests an older stellar population, exhibiting a yellowish-orange hue in the core region. The outer regions show a subtle decrease in color temperature. There are no prominent spiral arm structures or dust lanes visible. A slight elongation is observed, indicating a deviation from a perfectly circular form. No indications of any recent or major merger events can be observed in the image, but there is some very slight indication of minor disturbances in the outer regions. The galaxy appears relatively isolated.
