The galaxy exhibits an elliptical morphology with a high degree of central concentration. Its overall color appears slightly reddish, suggesting a population of older stars. The axial ratio indicates a flattening, but it is not significantly elongated. No distinct spiral arms or prominent dust lanes are apparent. There are no signs of any major ongoing merger events, although some minor disturbances may be present. The galaxy appears relatively smooth in texture, with a consistent color gradient from the core to the outer edges. The light distribution is somewhat asymmetric, implying a possible interaction or recent accretion event. The galaxy has a relatively low star formation rate.
