The galaxy appears as a relatively smooth, centrally concentrated object. It presents a slightly elliptical morphology, not perfectly spherical but also lacking a highly elongated shape. The light distribution shows a gradual decrease in intensity from the core outwards, with no distinct spiral arm features or prominent dust lanes visible in this image. There is a suggestion of a more compact, bright core region surrounded by a more diffuse halo. The overall color is somewhat blue-green, suggestive of the presence of some young, hot stars, however it is not a particularly active star forming galaxy. There are no clear signs of a major ongoing merger event, though there might be minor disturbances to the overall structure.
