The galaxy presents as a generally smooth object, elliptical in shape, with a distinct elongation. The color profile suggests a dominance of older stellar populations, exhibiting a yellowish-orange hue in the central region. This central area displays the highest surface brightness, gradually fading towards the outer edges. The lack of prominent spiral arms or dust lanes indicates a relatively quiescent system. There is some indication of blue light that has been detected, suggesting ongoing star formation at a low level. No major disturbances or signs of an ongoing merger are readily apparent from the image.
