The galaxy presents a primarily smooth and elliptical morphology. The light distribution suggests a relatively homogenous stellar population, with a high degree of central concentration. A faint, diffuse halo is visible, extending outwards from the bright central region. There appears to be minimal dust obscuration within the visible structure of the galaxy, giving it a relatively uniform color. There is a slight blue tint to the galaxy. No distinct spiral arms or bar structures are discernible, and no ongoing major merger events are evident from the image. However, there could be evidence of a minor disturbance. Overall, the galaxy appears to be a relatively quiescent system.
