The galaxy appears to be a relatively compact, elliptical system with a smooth, diffuse light distribution. Its color is largely yellow to orange, potentially indicating an older stellar population. There is a high degree of central concentration. Faint, diffuse light extends outward from the central region. No spiral arm structure is visible. The overall shape appears generally round with only a slight elongation. There is no sign of tidal tails, rings, or other strong indicators of a recent major merger event. A small degree of disturbance is possibly observed.
