The observed galaxy presents as a concentrated central bulge with a relatively smooth light distribution. There is a subtle disk-like structure that is barely visible surrounding this bulge. There appears to be some structural disturbance and light asymmetry. The appearance suggests the galaxy may be in the process of merging with another object. There is also a bright point like source that may or may not be a star cluster. It is difficult to see any arm structures or dust lanes in the image. The color of the galaxy appears to be reddish, suggesting older stellar populations dominate the light output. The relatively small apparent size and the faintness of the galaxy suggests a considerable distance.
