The galaxy appears as a relatively smooth, elliptical or lenticular system. Its light is concentrated in a central bulge region. The color is predominantly yellow-red, indicative of an older stellar population and potentially a lower rate of ongoing star formation. There is a slight indication of a faint disk component or extended halo. There does not seem to be evidence of a recent merger or major tidal disturbance, with most classifications leaning toward non-merging behavior.
