The galaxy presents as a relatively smooth, centrally concentrated object. It appears nearly circular, with a bright, ochre-colored core indicative of an older stellar population. Surrounding this core is a broader, less intense halo of greenish light. The overall color profile suggests a galaxy with ongoing, but limited, star formation occurring within its outskirts, while the core is dominated by more evolved stars. There are no obvious spiral arms or bar structures visible. No signs of recent major merger events or significant tidal disturbances are readily apparent. The light distribution seems quite symmetrical, consistent with a well-relaxed system.
