The galaxy presents as a somewhat diffuse object, exhibiting a generally elliptical morphology in its overall structure. There is evidence of a faint disk-like component with a slight inclination relative to our line of sight. The central region appears moderately brighter than the outer regions, suggesting a weak central bulge. There are possible signs of disturbance, such as faint tidal features in the outer regions. There is no strong indication of a significant merger event.
