The galaxy appears to be a large, relatively smooth, elliptical system exhibiting a dominant spheroidal component. It possesses a generally rounded shape, with a high degree of central concentration.

The galaxy's color is predominantly yellow-orange, suggestive of an older stellar population with lower levels of recent star formation. There is a secondary, smaller component that shows evidence of potential interaction or tidal disturbance. This feature is somewhat bluer in color, indicating a younger stellar population.

The primary body of the galaxy lacks any distinct spiral arm structure or prominent dust lanes. The light profile appears relatively smooth and featureless aside from some slight central diffraction. It appears to be undergoing a merger with a secondary, smaller galaxy.
