The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that graduates into a more diffuse surrounding halo. The light distribution suggests an older stellar population, with a color profile leaning towards the redder end of the spectrum. This indicates evolved stars dominating the galaxy's light output, possibly with ongoing, though relatively low levels of star formation. There is a subtle disk, but it doesn't appear to be a spiral galaxy. There does not appear to be any ongoing merging events.
