The galaxy appears as a centrally concentrated, relatively smooth object. The light distribution suggests a spheroid-dominated morphology, potentially an elliptical galaxy or a lenticular galaxy viewed face-on. There is a slight elongation, but overall, it appears fairly circular. The color is predominantly yellowish-orange, indicative of an older stellar population with relatively low levels of recent star formation and a higher proportion of evolved red giant stars. There is no obvious spiral structure or dust lanes visible. No signs of a major ongoing merger are evident, with a small chance of a minor disturbance being possible. The overall impression is a quiescent system.
