The galaxy presents as a relatively smooth, centrally concentrated object. The core region displays a bright, yellowish hue, suggesting an older stellar population. Fainter, bluer extensions can be seen surrounding the core, indicating the presence of some younger stars. The object exhibits a generally elliptical shape. There is a slight asymmetry visible, which might point towards a minor gravitational interaction or some internal disturbance. There is no distinct spiral arm structure, which would suggest the object is likely an elliptical galaxy.
