The galaxy appears as a single, relatively smooth object with an elliptical morphology. Color gradients are subtle, trending toward slightly redder hues at the core. The overall color suggests an older stellar population. There is no discernible dust lane or spiral arm structure. There is a low likelihood of the galaxy being involved in a major merger event. There may be evidence of minor disturbances to the central bulge, or perhaps a faint disk-like structure. Overall, the galaxy appears to be intermediate in size and mass and shows signs of low levels of star formation.
