The galaxy presents as a relatively compact, elliptical morphology. It exhibits a high degree of central concentration, appearing smooth with no discernible spiral arm structures or significant dust lanes. The light profile is consistent with an early-type galaxy. There is little evidence of recent or ongoing star formation. The color is generally redder, suggesting an older stellar population and a lack of significant blue light from young, massive stars. There is a faint tidal tail on one side, suggesting a past minor disturbance.