The galaxy appears to be an elliptical galaxy, or at least a smooth, early-type galaxy, with a dominant, spheroidal component. It exhibits a high degree of central concentration, indicated by a bright, compact core region that gradually fades outwards. The light distribution is generally smooth and symmetrical. The galaxy has an overall circular shape. There is little to no evidence of spiral arms or other disk-like features. Faint blue light is present, especially in the outer regions of the galaxy, suggesting a small amount of ongoing star formation. There is no clear sign of any major mergers or significant tidal disturbances. Overall, the morphology suggests a relatively evolved and quiescent system.
