The galaxy appears as a well-defined, elliptical structure. It presents a generally smooth texture and a symmetrical, rounded shape. The central region shows a concentration of light, potentially indicating a bulge component. While the galaxy exhibits an overall homogenous appearance, a slight color gradient exists. The core appears slightly redder compared to the outer regions, which exhibit a bluer hue. This color difference suggests varying stellar populations and ongoing star formation activity. The galaxy exhibits a minor disturbance. No prominent spiral arms or bars are discernible, and the overall morphology suggests a relatively evolved system.
