The galaxy presents as a fairly compact elliptical system. It exhibits a smooth, diffuse light profile without any discernible spiral arm structures or prominent dust lanes. The light is concentrated toward the center, with a gradual decrease in intensity outwards. The galaxy appears nearly circular. The color profile indicates a dominant population of older stars, lending a yellowish hue to the galaxy’s overall appearance. There are no obvious signs of recent major merger activity. The overall appearance suggests a relaxed system that is undergoing relatively little star formation at the current epoch.
