The galaxy presents a generally smooth morphology, exhibiting a centrally concentrated luminosity profile. Its shape appears approximately round, lacking any obvious strong asymmetries or spiral arm structures. The galaxy displays a yellow-white hue, suggesting a stellar population dominated by older, evolved stars. There is a hint of bluer light in the outskirts, potentially indicative of some ongoing, albeit minimal, star formation activity. The system does not obviously show any signs of a major merger event, although there could be some subtle indications of minor tidal disturbances.
