The galaxy presents as a relatively smooth, elliptical-like structure. There is a high degree of central concentration of light, giving it a bright core. The light appears to fade gradually from the center outwards. There is a slight elongation in the overall shape of the galaxy. There is no apparent spiral structure or significant dust lanes visible. The galaxy's color suggests an older stellar population with a general lack of ongoing star formation. It does not appear to be undergoing any major merging activity, although there is a very slight asymmetry which may be due to a minor interaction.
