The galaxy presents as a single, relatively smooth object. It is generally elliptical in shape, with a high degree of circularity. There is a central concentration of luminosity that gradually fades into the outer regions of the galaxy. The light appears to be generally white, perhaps with a slightly red hue, indicating an older stellar population. There is no apparent disk structure, spiral arms, or significant dust lanes visible in this image. There is no sign of any major disturbance or merger. There may be some slight evidence of tidal streams around the galaxy, or potentially another, smaller galaxy in the process of merging.
