The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is primarily spheroidal, appearing nearly round but with a slight elongation. No distinct features such as spiral arms, bars, or prominent dust lanes are discernible in this image. The color gradient suggests a concentration of older stellar populations, with a yellowish hue dominating the central region of the galaxy. There is no evident disturbance in its structure indicative of a recent major merger event. The galaxy appears to be relatively isolated.
