The galaxy presents as a smooth, elliptical-like structure. The light distribution is centrally concentrated, with a gradual decrease in luminosity outwards. The core appears yellowish, potentially indicating an older stellar population. The galaxy does not exhibit any prominent spiral arm structure or distinct features such as dust lanes. A slight elongation is visible, deviating from a perfectly circular shape. No signs of major mergers or significant tidal disturbances are apparent. Overall, the galaxy has a relatively quiescent appearance.
