The galaxy appears to be a relatively smooth, elliptical galaxy. The color distribution suggests an older stellar population, with a dominant yellowish hue in the central region. There is a slight radial decrease in the luminosity profile. The isophotes appear generally round. There is no apparent evidence of spiral arms or significant dust lanes. There may be a subtle hint of a diffuse halo, but its boundaries are difficult to discern against the background noise. Overall, the galaxy exhibits characteristics consistent with an early-type galaxy undergoing minimal recent star formation. The object does not appear to be undergoing any major mergers or tidal disturbances.
