The galaxy presents as a centrally concentrated, relatively smooth object. It is elliptical in shape, displaying a fairly even light distribution without significant spiral arm structures or prominent dust lanes visible. The color profile is relatively uniform, with a slightly bluer hue in the central region, possibly indicating a population of younger, hotter stars, and an overall decrease in blue light as you move towards the outer edges. The galaxy exhibits a general lack of strong features indicative of active star formation, such as HII regions or distinct knots of blue light. There are no obvious signs of tidal tails, rings, or morphological distortions suggesting a recent major merger event. The overall appearance suggests a system dominated by an older stellar population and exhibiting minimal ongoing star formation activity. Some minor disturbances cannot be ruled out, but based on the image, this is likely a relatively relaxed and undisturbed system.
