The galaxy presents as a generally smooth, elliptical structure. It appears to be in the shape of a disc or oval, with a bright, concentrated central bulge. The primary color is a soft white, indicating an older stellar population within the bulge. Emanating from the central bulge is a more diffuse halo showing hints of blue, with a significant fraction that is smoothly distributed, which could imply the presence of a small disk. The outer regions of the galaxy exhibit some hints of disk morphology. There also appears to be only minor disturbances visible, indicating a low rate of mergers or interactions with other galaxies. There are small traces of features such as spiral arms, or irregular patches indicating on-going or recent episodes of star formation, which accounts for the blue light present in the halo. These features are small, and the main impression is that of a relatively quiescent galaxy. The overall color gradients suggest a range of stellar ages, where the central bulge is significantly redder than the halo and outer regions. The light is relatively uniform across the body of the galaxy.
