The galaxy appears as a single, smooth concentration of light, generally elliptical in shape. It is a bright yellowish/orange hue, implying an older stellar population with a relatively low rate of star formation, and may be dominated by evolved stars. The galaxy's light profile seems to be fairly uniform across its body, with no indication of spiral arms or other distinct morphological features. There is no obvious sign of any significant tidal disturbances or mergers affecting the galaxy's structure. The galaxy appears to be a fairly massive system.
