The galaxy presents as a relatively smooth, elliptical morphology. It appears to be somewhat spheroidal with a high degree of central concentration and an absence of any prominent disk-like structure or spiral arms. The color is generally redder, indicating an older stellar population and a suppressed rate of recent star formation. The light profile suggests a generally uniform decline in luminosity from the core outward. There is no evidence of ongoing major mergers or tidal distortions, though some minor disturbances cannot be entirely ruled out. The galaxy is fairly compact in physical size, given its apparent distance.
